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      Astrogeophysics: T.G. Barnes, D.Sc.; H.S. Slusher Ph.D., D.Sc.; C.A. Paiva, M.S.
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  <p id="description">[PLEASE USE CONTROL (+) FOR ZOOM AND CONTROL (0) FOR NORMAL VIEW].To see other BSMRA sites the BSM Research Associates Integrated Websites Selection.   Also please use the included PDFs and WORD files for higher resolution if desired. With regards to doppler interpretation for spectral absorption and emission lines, it is not possible for electromagnetic waves to propagate through interstellar and 
intergalactic space (filled with hydrogen and helium transmission fields) without substantial loss of amplitude and wavelength.  The assumption of an expanding universe based on the doppler interpretations of spectral redshifts is, due to the ignoring of the propagation physics resulting in absorption and scattering by interplanetary, interstellar, intergalactic and inter-galactic cluster transmission fields.
As the tension of the universe decreases (in accordance with the Second Law of Thermodynamics) the square root of the ratio of tension-to-density (i.e. velocity of light) also decreases.  Another result is the elongation
of electromagnetic wave propagation falsely interpreted as a doppler velocity shift.  Stretching universe field lines increase tension which result in an increase of total electromagnetic frequency and 
decrease of wavelengths observed, while decreased tension has the opposite effect
So-called emission and absorption spectral "reddening" effects are really
functions of electromagnetic re-emission at longer wavelengths.  The electromagnetic wavelength increases are not the result of a doppler velocity effects, but rather physical electro-optical
results.  The electromagnetic extinction in intergalactic and inter-galactic cluster space is the result of the characteristics of the intergalactic and inter-galactic cluster transmission fields.  Super-galactic cluster collisions occurring along Geller Shocks Zones (GSZ) generate 
exceedingly high intergalactic temperatures, and result in the generation of gamma and X-rays.  These high-frequency transmission fields further affect the intergalactic transmission field's propagation characteristics to the extent that extinction is increased through interference.  Galaxies of 
super clusters forming around Geller Shock Zones are 
located within 100 million-degree Celsius hydrogen and helium gas 
clouds.  These intergalactic gas clouds absorb, scatter and re-transmit radiation, the propagation of which includes light 
(.398 -. 780 microns). This generates the impression of velocity doppler effects, and yet has nothing 
to do with assumed galaxy expansion processes.  For example concentrations of 10-20 million-degree gas fields have been 
observed surrounding large galaxies clusters of NGC 4889 and NGC 4874, resulting in an incorrect assumption of doppler velocities to spectral line shifts; such line shifting being functions of transmission through
very hot hydrogen and helium intergalactic space near galaxy cluster compression zones.  

The images shown below from Dr. Halton Arp's catalogue and re-processed here (BSM Research Associates) reveal galaxy disintegration processes, which further add to the intergalactic dust and the hydrogen-helium gas fields within galactic clusters.  Galaxies are always in clusters of galaxies found along Geller nodal compression
zones. An expanding universe model is proven neither by astrophysical field data, nor by electromagnetic propagation physics. 
Electromagnetic absorption, scattering and re-transmission of radiation in the REAL universe are based on a decreasing Integrated Field System (IFS) line tension.  This results in a reduction in cumulative observed wavelengths across broadband transmission.  Another caution:  Earth is neither at the center of the Solar System nor at the center of this galaxy. 
THIS SITE ALSO INCLUDES THE UNIVERSITY OF TEXAS AT EL PASO (PHYSICS DEPARTMENT) THOMAS G. BARNES AND HAROLD S. SLUSHER FILES
KEYS: Messier 66  M65; Arp 317

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     <h2 class="date-header">Tuesday, 09 February 2010</h2>
      
   <div class="post"><a name=33></a>
    <h3 class="post-title">Full Translation of this Site</h3>
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      <p><P><A href="http://www.freetranslation.com/"></A><STRONG>&nbsp;</STRONG><A href="http://www.freetranslation.com/"><STRONG><FONT size=4>Full Translation</FONT></STRONG></A><STRONG>: Steps: (1.) Press Full Translation; (2.) <EM>Select Web Translation</EM>; (3.) Copy and paste: </STRONG><A href="http://smtp.antelecom.net/blogs/bsmaastrophysics/"><STRONG>http://smtp.antelecom.net/blogs/bsmaastrophysics/</STRONG></A><STRONG>&nbsp;into the&nbsp;white box section and be sure to select your language.</STRONG></P>
<P><STRONG>(<A href="http://smtp.antelecom.net/blogs/BSMRAMainsite/">BSMA Main Site</A>)</STRONG></P>
<P><A href="http://www.google.com/search?q=Clifford+A.+Paiva+BSMRA&amp;hl=en&amp;filter=0"><STRONG>[All BSMRA Sites]</STRONG></A><BR><A href="http://www.freetranslation.com/"></A>&nbsp; <BR><A href="http://www.freetranslation.com/"><IMG src="a_33_SDL_Translation_Box.jpg"></A>&nbsp;</P>
<P><A href="a_33_Clifford_Anthony_Paiva_RESUME__2010.doc"><STRONG>Clifford Anthony Paiva RESUME 2010.doc</STRONG></A> </P></p>
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      <em>Clifford A. Paiva @ 09:27 AM</em>
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     <h2 class="date-header">Saturday, 31 October 2009</h2>
      
   <div class="post"><a name=32></a>
    <h3 class="post-title">Clifford Anthony Paiva_BSMRA:  Single Background Frame for BSMRA_Fomalhaut Star System Used TWICE; BSMRA_Fomalhaut B; Accumulation Dust Zone Centers (DZC); HR 8799 DZCs and Not  Yet Confirmed Planets Without Assumptions Implemented</h3>
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      <p><P style="TEXT-ALIGN: justify"><SPAN style="mso-bidi-font-size: 9.0pt"><SPAN style="COLOR: red"><SPAN style="mso-spacerun: yes"></SPAN></SPAN></SPAN></P>
<P><A href="http://smtp.antelecom.net/blogs/BSMRAMainsite/"><STRONG>BACK TO BSMRA MAIN SITE</STRONG></A></P>
<P><A href="http://hubblesite.org/newscenter/archive/releases/2008/39/"><STRONG>Hubble Space Telescope has imaged Fomalhaut</STRONG> </A><STRONG>interstellar dust accumulation centers, currently are assumed to be planets (i.e. Fomalhaut B).&nbsp;&nbsp;A very close examination of the Fomalhaut&nbsp;interplanetary dust system reveals, as indicated in the BSM Research imagery presented in this section, multiple infrared accumulation dust zones (ADZs). It is the differential velocity components of the orbiting dust field around the Fomalhaut star, allegedly out of which an assumed planet (Fomalhaut B), is assumed to have acretted from the ambient dust field.&nbsp; Here it should be noted that outward pressure constraints and entropy produced by processes associated with&nbsp;the Second Law of Thermodynamics, precludes the possibility of&nbsp;<EM><U>any</U></EM> planet forming from an interplanetary&nbsp;dust field.&nbsp; In any case in a two year elapse&nbsp;a differential orbiting dust field arount the Fomalhaut star should have occurred, yielding differential changes in intensity; spatially and spectrally.&nbsp; Further the nearby interstellar area around Fomalhaut reveals an intense interstellar gas and dust vortex <U><EM>wake</EM></U>.&nbsp; Yet the two frames used by NASA, allegedly two year apart to indicate planetary displacement, are pixel-by-pixel, precisely identical.</STRONG></P>
<P><A href="http://homepages.inf.ed.ac.uk/rbf/HIPR2/pixsub.htm"><STRONG>BSMR_</STRONG><STRONG>Fomalhaut B Interstellar Dust System.doc</STRONG></A> </P>
<P><A href="http://smtp.antelecom.net/blogs/bsmaastrophysics/a_32_Fomalhaut_Addition_Accumulation_Dust_Centers.doc"><STRONG>BSMR_</STRONG><STRONG>Fomalhaut Addition Accumulation Dust Centers.doc</STRONG></A>&nbsp;</P>
<P><STRONG>A single&nbsp;frame revealing&nbsp;an orbiting dust field background around the Fomalhaut star&nbsp;, was used twice by NASA;&nbsp;indicating </STRONG><STRONG>possible science fraud</STRONG><STRONG>.&nbsp; <U>Temporal backgrounds do not, over large observation times ( two years) result in zero changes in intensities (spectrall and spatially</U>).&nbsp; Yet the background frames for the planet Fomalhaut B displacements, when subtracted, are exactly zero in intensity...indicating the same frame was subtracted from itself resulting in the zero intensity value.</STRONG></P>
<P><STRONG><U>Electro-Optics and Infrared</U> <U>Notes Concerning Orbiting Thermal Dust Fields</U>: </STRONG></P>
<P><STRONG>Two&nbsp;years (2004-2006) observation&nbsp;elapse time&nbsp;would have changed stellar dust fields' intensity levels spatially, spectrally and temporally (SST) along the line-of-sight from the Earth to Fomalhaut B.&nbsp; This occurs as a function of, among other significant factors,&nbsp;Fomalhault star SST interstellar displacement and intensity variations (note frame above indicating interstellar displacement wake).&nbsp; This same propagation&nbsp;physics&nbsp; is applied to our solar system's&nbsp;SST variations for the sun,&nbsp;its interplanetary dust field, and&nbsp;its interstellar dust field line-of-sight (LOS), all the way to&nbsp;the Fomalhaut System some 25-30 light years distance.</STRONG>&nbsp;&nbsp;<STRONG><U>However</U></STRONG>&nbsp;<U><STRONG>NO variations</STRONG></U> <STRONG>are observed for the two background dust field frames used by <A href="http://www.solarviews.com/eng/fomalhaut.htm">NASA Goddard Space Flight Center Fomalhaut Team</A> after <A href="http://homepages.inf.ed.ac.uk/rbf/HIPR2/pixsub.htm">image subtraction</A>; pixel-by-pixel assessed at BSMRA.&nbsp; In any case both frames for thermal dust field backgrounds are</STRONG> <STRONG><EM><U>identical</U></EM></STRONG>,<STRONG> <U><EM>pixel-by-pixel</EM></U>: <U><EM>spatially, spectrally and in intensity</EM></U>.&nbsp; Hence a</STRONG> <STRONG><EM><U>single frame was used at least twice.</U>&nbsp; </EM>Notice that while the black arrow target planet designation moves spatially and in intensity in 3D imagery, the background 3D intensity (and its pixel spatial and temporal (2-year) characteristics) change is <U>zero</U>.&nbsp; Of course if the same frame is used twice, zero changes in pixels SST is expected; and zero changes are&nbsp;here observed.</STRONG></P>
<P><A href="http://smtp.antelecom.net/blogs/BSMRAMainsite/"><STRONG>BACK TO BSMRA MAIN SITE</STRONG></A><BR><A href="http://homepages.inf.ed.ac.uk/rbf/HIPR2/pixsub.htm"><STRONG>BSMRA_</STRONG><STRONG>Fomalhaut Background Image Subtraction Should Not Be Zero.doc</STRONG></A> </P>
<P><A href="http://smtp.antelecom.net/blogs/bsmaastrophysics/a_32_Cliff_PRIMARY_Prime_Military__RESUME__2009.doc"><STRONG>BSMRA_</STRONG><STRONG>Clifford Anthony Paiva RESUME 2009.doc</STRONG></A></P>
<P><A href="http://smtp.antelecom.net/blogs/bsmaastrophysics/a_32_Identical_Background_Used_Twice_by_NASA_Fomalhaut_Team.doc"><STRONG>BSMRA_</STRONG><STRONG>Identical Background Used Twice by NASA Fomalhaut Team.doc</STRONG></A><STRONG> <BR></STRONG><A href="http://smtp.antelecom.net/blogs/bsmaastrophysics/a_32_Identical_Background_Used_Twice_by_NASA_Fomalhaut_Team.doc"><IMG src="a_32_Fomalhaut_Identical_Frames_Used_Twice_out_1.jpg"></A>&nbsp;<A href="http://smtp.antelecom.net/blogs/bsmaastrophysics/a_32_Identical_Background_Used_Twice_by_NASA_Fomalhaut_Team.doc"><IMG src="a_32_Fomalhaut_Identical_Frames_Used_Twice_out_2.jpg"></A> <A href="http://smtp.antelecom.net/blogs/bsmaastrophysics/a_32_Identical_Background_Used_Twice_by_NASA_Fomalhaut_Team.doc"><IMG src="a_32_Fomalhaut_Identical_Frames_Used_Twice_out_3.jpg"></A> <A href="http://smtp.antelecom.net/blogs/bsmaastrophysics/a_32_Identical_Background_Used_Twice_by_NASA_Fomalhaut_Team.doc"><IMG src="a_32_Fomalhaut_Identical_Frames_Used_Twice_out_4.jpg"></A> <A href="http://smtp.antelecom.net/blogs/bsmaastrophysics/a_32_Identical_Background_Used_Twice_by_NASA_Fomalhaut_Team.doc"><IMG src="a_32_Fomalhaut_Identical_Frames_Used_Twice_out_5.jpg"></A> <A href="http://homepages.inf.ed.ac.uk/rbf/HIPR2/pixsub.htm"><IMG src="a_32_Fomalhaut_Identical_Frames_Used_Twice_out_6.jpg"></A> </P><A href="a_32_BSMRA_Arp_Objects_in_Arp_and_NGC_Sequence.pdf"><STRONG>BSMRA_Arp Objects in Arp and NGC Sequence.pdf</STRONG></A> </p>
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      <em>Clifford A. Paiva @ 15:13 PM</em>
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		  			<div class="comment-body"><a name=32_1></a>
			  <p><b>Cliff:</b> People are exceedingly fast in pre-identifying assumed exo-planets. A case in point is the Fomalhaut System with supposedly 2 planets. In fact as identified here, <STRONG><EM><U>many</U></EM></STRONG> accumulaiton dust zones (ADCs) are present in the Fomalhaut System, and of course these cannot all be planets. Dust accredtion into planets is an evolution concept and entirely scientifically untenable due to thermodynamic constraints of gravitional compression and entropy restrictions.&nbsp; Also folks must&nbsp;assume the existence of evolution to ascribe life on other planets, if in fact other planets do exist; the incredibly complex design of biochemical and molecular biological systems doesn't appear to bother them. Life IS out there of course...He has always been out there and here. God is not a religion but a Person and any attempt to extricate Him from science results in very deficient investigations.&nbsp; Another case in point is the ship at the 16,300 foot altitude on Mt. Ararat, and a completely fracture lithosphere (crust) predominantly sedimentary (<STRONG><EM><U>sediment</U></EM></STRONG>) in origin. <small>(10/31/09)</small></p>
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		  			<div class="comment-body"><a name=32_2></a>
			  <p><b>Cliff:</b> HR 8799 is calculated to be 130 light years with three accumulation dust centers (ADCs).  Fomalhaut is determined to be 25 light years with one confirmed ADC. Both are pictured together on above frames.  The former is an IR composite; the latter an optical (visual) bandpass frame. <small>(11/02/09)</small></p>
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		  			<div class="comment-body"><a name=32_3></a>
			  <p><b>Cliff:</b> The giant interstellar gas-dust vortex wake of Fomalhaut indicates intense dislacement through interstellar space. Fomalhaut internal stability is affected by the angular displacment as revealed in the gas wake. (11/03/09) <small>(11/03/09)</small></p>
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		  			<div class="comment-body"><a name=32_4></a>
			  <p><b>Cliff:</b> Image subtraction should not be zero, but rather some value above zero (for absolute subtraction).&nbsp; In fact the background frames are exactly zero which indicates the same background frame was used to indicate a target (planet Fomalhaut B) displacement; not two frames taken over&nbsp;2 years apart (2004 and 2006). &nbsp;Again: Only a single frame&nbsp; was used for both&nbsp;Fomalhault B's backgrounds. It is promulgated on the internet that the Fomalhaut B planet is moving with respect to <EM><STRONG><U>two</U></STRONG></EM> frames. However the same background frame is used <STRONG><EM><U>twice</U></EM></STRONG>. The implications for scientific fraud is direct, since background stellar dust fields (interplanetary dust) shuld be in orbit around the host star; changing in intensity, spectrally and spatially.&nbsp;&nbsp;Two stellar systems, in addition to the line-of-sight propagation distance,&nbsp;in this case to the Fomalhaut&nbsp;System, is involved.&nbsp; Variations over a two year period are expected....none is revealed in the background thermal dust imagery.&nbsp;(11/05/09) <small>(11/05/09)</small></p>
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     <h2 class="date-header">Monday, 31 August 2009</h2>
      
   <div class="post"><a name=31></a>
    <h3 class="post-title">Clifford Anthony Paiva_BSMRA:  Stardust Mission Integrity Questions: The Isotopic Abundance of Glycine-Carbon-13 On Earth and Mission Contamination</h3>
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      <p><P style="TEXT-ALIGN: justify"><SPAN style="COLOR: #4b5c68"><STRONG><A href="http://smtp.antelecom.net/blogs/BSMRAMainsite/">Back to BSMRA Main Site</A></STRONG></SPAN></P>
<P style="TEXT-ALIGN: justify"><SPAN style="COLOR: #4b5c68">Earlier, preliminary analysis in the NASA Goddard labs detected glycine in both the <STRONG><EM><U>foil</U></EM></STRONG> </SPAN><B><SPAN style="COLOR: red">(BSMRA: this is <U>contamination</U> since glycine molecules would have been vaporized on impact with the aluminum wall, which is of course the reason for the requirement of the aerogel on the STARDUST mission)</SPAN></B><SPAN style="COLOR: #4b5c68"> and a sample of the aerogel. However, since glycine is used by <I>terrestrial</I> life, at <B><I><U><A href="http://stardust.jpl.nasa.gov/news/news115.html">first the team was unable to rule out contamination from sources on Earth. "It was possible that the glycine we found originated from handling or manufacture of the Stardust spacecraft itself,"</A></U></I></B> said Elsila (NASA-Astrobiology). The new research used isotopic analysis of the <STRONG><EM><U>foil</U></EM></STRONG> </SPAN><B><SPAN style="COLOR: red">(BSMRA: aluminum)</SPAN></B><SPAN style="COLOR: #4b5c68"> to rule out </SPAN><B><SPAN style="COLOR: red">(BSMRA: this is an unwarranted assumption since 1.1% of carbon on Earth <I>IS</I> <SUP>13</SUP>C)</SPAN></B><SPAN style="COLOR: #4b5c68"> that possibility.<BR><BR><SPAN style="mso-spacerun: yes">&nbsp;</SPAN>…A glycine molecule from space will tend to have more of the heavier Carbon-13 atoms in it than glycine that's from Earth </SPAN><B><SPAN style="COLOR: red">(BSMRA: Incorrect since displacement through the solar plasma field (solar wind) precludes the possibility of any intact glycine. Any Carbon 13 within the solar wind plasma field would be dissociated into its atomic constituents; not remaining in glycine</SPAN></B><SPAN style="COLOR: #4b5c68"> </SPAN><B><SPAN style="COLOR: red">form.)</SPAN></B><SPAN style="COLOR: #4b5c68"> That is what the team found. </SPAN><B><SPAN style="COLOR: red">(BSMRA: The NASA astrobiology team found 13C contamination)</SPAN></B><SPAN style="COLOR: red">.<?xml:namespace prefix = o ns = "urn:schemas-microsoft-com:office:office" /><o:p></o:p></SPAN></P>
<P><SPAN style="FONT-FAMILY: 'Times New Roman'; COLOR: #4b5c68; FONT-SIZE: 12pt; mso-fareast-font-family: 'Times New Roman'; mso-ansi-language: EN-US; mso-fareast-language: EN-US; mso-bidi-language: AR-SA"><SPAN style="mso-spacerun: yes">&nbsp;</SPAN>"We discovered that the Stardust-returned glycine has an </SPAN><I><SPAN style="FONT-FAMILY: 'Times New Roman'; FONT-SIZE: 12pt; mso-fareast-font-family: 'Times New Roman'; mso-ansi-language: EN-US; mso-fareast-language: EN-US; mso-bidi-language: AR-SA">extraterrestrial</SPAN></I><B><SPAN style="FONT-FAMILY: 'Times New Roman'; COLOR: red; FONT-SIZE: 12pt; mso-fareast-font-family: 'Times New Roman'; mso-ansi-language: EN-US; mso-fareast-language: EN-US; mso-bidi-language: AR-SA"> (BSMRA: another NASA assumption)</SPAN></B><SPAN style="FONT-FAMILY: 'Times New Roman'; COLOR: #4b5c68; FONT-SIZE: 12pt; mso-fareast-font-family: 'Times New Roman'; mso-ansi-language: EN-US; mso-fareast-language: EN-US; mso-bidi-language: AR-SA"> carbon isotope signature, indicating that it originated on the comet," said Elsila. </SPAN><B><SPAN style="FONT-FAMILY: 'Times New Roman'; COLOR: red; FONT-SIZE: 12pt; mso-fareast-font-family: 'Times New Roman'; mso-ansi-language: EN-US; mso-fareast-language: EN-US; mso-bidi-language: AR-SA">Elsila is not admitting an otherwise <U>mishandled</U> experiment via unnecessary contamination of the STARDUST mission, and attempting to turn the mistake to the benefit NASA; essentially by covering a contamination occurrence of a multi-million dollar NASA effort. </SPAN></B><B><SPAN style="FONT-FAMILY: 'Times New Roman'; COLOR: red; FONT-SIZE: 12pt; mso-fareast-font-family: 'Times New Roman'; mso-ansi-language: EN-US; mso-fareast-language: EN-US; mso-bidi-language: AR-SA">[Further Interest: </SPAN></B><STRONG><FONT color=#ff0000><A href="http://smtp.antelecom.net/blogs/bsmaCIA/">http://smtp.antelecom.net/blogs/bsmaCIA/</A>]</FONT></STRONG></P>
<P><A href="http://stardust.jpl.nasa.gov/home/index.html"><IMG src="a_31_NASA_Stardust_Contamination.jpg"></A>&nbsp;<BR><STRONG>Clifford A. Paiva_</STRONG><A href="http://smtp.antelecom.net/blogs/bsmaastrophysics/a_31_Stardust_Contamination_BEFORE.doc"><STRONG>BSMRA_Stardust Contamination BEFORE.doc</STRONG></A><STRONG> </STRONG></P>
<P><A href="http://smtp.antelecom.net/blogs/bsmaastrophysics/a_31_Intergalactic_Dust.pdf"><STRONG>BSMRA_</STRONG><STRONG>Intergalactic Dust.pdf</STRONG></A> </P>
<P><A href="a_31_Cliff_PRIMARY_Prime_Military__RESUME__2009.doc"><STRONG>Clifford Anthony Paiva RESUME 2009.doc</STRONG></A><STRONG> <BR></STRONG><BR><A href="http://dynamics.chem.ox.ac.uk/projects/project1.html"><IMG src="a_31_Solar_Wind_PD_out_1.jpg"></A> <BR><A href="http://dynamics.chem.ox.ac.uk/projects/project1.html"><IMG src="a_31_Solar_Wind_PD_out_2.jpg"></A>&nbsp;<BR><STRONG>Clifford A. Paiva_</STRONG><A href="http://smtp.antelecom.net/blogs/bsmaastrophysics/a_31_Photodissociation_of_Peptide_Model_Compounds_out1.doc"><STRONG>BSMRA_Photodissociation of Peptide Model Compounds out1.doc</STRONG></A></P>
<P><STRONG>Clifford A. Paiva_<A href="http://s8int.com/phile/page62.html">BSMRA</A></STRONG>_<A href="http://s8int.com/phile/page62.html"><STRONG>SI8 and Interplanetary Dust</STRONG></A></P>
<P><STRONG><A href="http://www.google.com/search?q=Clifford+A.+Paiva+BSMRA&amp;hl=en&amp;filter=0">All BSMRA Sites</A></STRONG></P></p>
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      <em>Clifford A. Paiva @ 09:49 AM</em>
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			  <p><b>Cliff:</b> No apologies here from BSM Research since NASA has no apologies regarding the unecessary contamination of a 150 million dollar mission, probably before the STARDUST satellite even left the laboratory. <small>(08/31/09)</small></p>
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     <h2 class="date-header">Monday, 24 August 2009</h2>
      
   <div class="post"><a name=30></a>
    <h3 class="post-title">Clifford Anthony Paiva_BSMRA:  Disintegration of Vortex Galaxies; So-Called "Quasars":  Normal Stars and Galaxies; Dr. Halton Arp (Max Planck Institute); Assumed Doppler Interpretation for Redshift and Application Within the BSMRA_Hubble Constant; Closed Science</h3>
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<P><A href="http://haysvillelibrary.files.wordpress.com/2009/05/galaxies-on-collision-course-hst-ultra-deep-field.jpg"><STRONG>BSMRA_Galaxies are exceedingly high-entropy vortex systems in the process of <EM>disintegration</EM></STRONG></A><STRONG>;</STRONG> not formation.&nbsp; Further&nbsp;stars within dense interstellar (intra-galactic) dust&nbsp;transmission fields, and galaxies within intergalactic cluster fields;&nbsp;absorb, multiple-scatters, and re-transmits electromagnetic radiation at all wavelengths, but particularly at in the .398-.780 micron and shorter propagation bandpasses. Extinction and reddening increases as a function of decreasing wavelength resulting in percieved spectral shifts.&nbsp;Also the <EM>intensity</EM> and of re-emitted radiation is specific to the characteristics of the interstellar dust and gas fields, intergalactic and inter-cluster (between galactic clusters) and&nbsp;along acoustic (<A href="http://www.cfa.harvard.edu/~mjg/">Geller)</A> field zones.&nbsp;&nbsp; The <STRONG>X-ray QSO (X-QSO)</STRONG> has been measured by <A href="http://chandra.harvard.edu/"><STRONG>CHANDRA X-ray</STRONG> </A>observations: 1.5(10)^40 erg/s. Such prodigious amounts of very short wave electromagnetic wave propagation energy is subject to absorption and multiple-scattering by interstellar (ISM), inter-galactic, intra-cluster&nbsp;(IGM, <A href="http://en.wikipedia.org/wiki/Intracluster_medium">ICM</A>)&nbsp;and inter-galactic cluster (IGCM)&nbsp;transmission&nbsp;media. <A href="http://wiki.answers.com/Q/What_is_the_wavelength_of_an_X-ray"><STRONG>X-ray</STRONG> </A>sources are subject to intense extinction by&nbsp;&nbsp;<A href="http://en.wikipedia.org/wiki/Cosmic_dust">ISM</A>, and <A href="http://en.wikipedia.org/wiki/Intracluster_medium">extremely hot IGM, and ICM </A>transmission fields. More data is included from <A href="http://iso.esac.esa.int/">Infrared Space Observatory (ISO) </A>, <A href="http://www.spitzer.caltech.edu/Media/mediaimages/zooms/index.shtml">Spitzer Space Telescope (SST)</A> and its <A href="http://www.iop.org/EJ/article/0067-0049/154/1/18/60259.web.pdf?request-id=9a78e440-acc8-43d9-acbe-3ec73c4aaf2d">Infrared Spectrograph (IRS).</A> Other&nbsp;space <A href="http://www.spitzer.caltech.edu/">electro-optics&nbsp;programs </A>are included in this section.<A href="a_30_Quasars_So-Called_Are_In_Fact_Normal_Stars_and_Galaxies.pdf">Quasars So-Called Are In Fact Normal Stars and Galaxies.pdf</A>.&nbsp; <STRONG><A href="http://nedwww.ipac.caltech.edu/level5/Arp/Arp_contents.html">Dr. Halton Arp's Peculiar Galaxy Catalogue</A></STRONG>.<BR><BR><A href="http://smtp.antelecom.net/blogs/bsmaastrophysics/a_30_Redshift_As_A_Function_of_Electromagnetic_Wave_Absorption__Scattering_and_Re-Transmission.pdf"><IMG src="a_30_Xray_Seyfert_II_NGC_7319_X-QSO.jpg"></A>&nbsp;</P>
<P><A href="http://smtp.antelecom.net/blogs/bsmaastrophysics/a_30_Redshift_As_A_Function_of_Electromagnetic_Wave_Absorption__Scattering_and_Re-Transmission.pdf"><STRONG>BSMRA_Redshift As A Function of Electromagnetic Wave Absorption, Scattering and Re-Transmission.pdf</STRONG></A> <BR><A href="http://smtp.antelecom.net/blogs/bsmaastrophysics/a_30_Redshift_As_A_Function_of_Electromagnetic_Wave_Absorption__Scattering_and_Re-Transmission.pdf"><STRONG>BSMRA_Interstellar and IGM dust Primary.doc</STRONG></A><STRONG>&nbsp;<A href="http://smtp.antelecom.net/blogs/bsmaastrophysics/a_30_Clerk-Maxwell_Moving_Field_Equations.doc">BSMRA_</A></STRONG><STRONG><A href="http://smtp.antelecom.net/blogs/bsmaastrophysics/a_30_Clerk-Maxwell_Moving_Field_Equations.doc">Clerk-Maxwell Moving Field Equations.doc</A></STRONG> <BR><A href="http://smtp.antelecom.net/blogs/bsmaastrophysics/a_30_Redshift_As_A_Function_of_Electromagnetic_Wave_Absorption__Scattering_and_Re-Transmission.pdf"><IMG src="a_30_Hubble_Constant_Assumed.jpg"></A> <BR><A href="http://smtp.antelecom.net/blogs/bsmaastrophysics/a_30_Redshift_As_A_Function_of_Electromagnetic_Wave_Absorption__Scattering_and_Re-Transmission.pdf"><IMG src="a_30_Hubble_Constant_Assumed2_.jpg"></A> <BR><A href="http://smtp.antelecom.net/blogs/bsmaastrophysics/a_30_Clerk-Maxwell_Moving_Field_Equations.doc"><IMG src="a_30_Hubble_Constant_Assumed3_.jpg"></A> <BR><A href="http://smtp.antelecom.net/blogs/bsmaastrophysics/a_30_Clerk-Maxwell_Moving_Field_Equations.doc"><IMG src="a_30_Hubble_Constant_Assumed4.jpg"></A> <BR><A href="http://smtp.antelecom.net/blogs/bsmaastrophysics/a_30_Electromagnetic_Extinction_From_Interstellar_Dust.doc"><STRONG>BSMRA_</STRONG><STRONG>Electromagnetic Extinction From Interstellar Dust.doc</STRONG></A><STRONG> <BR><A href="http://smtp.antelecom.net/blogs/bsmaastrophysics/a_30_EXTINCTION_AS_A_FUNCTION_OF_PARTICLE_DIAMETER.doc">BSMRA_</A></STRONG><STRONG><A href="http://smtp.antelecom.net/blogs/bsmaastrophysics/a_30_EXTINCTION_AS_A_FUNCTION_OF_PARTICLE_DIAMETER.doc">EXTINCTION AS A FUNCTION OF PARTICLE DIAMETER.doc</A></STRONG> <BR><A href="http://smtp.antelecom.net/blogs/bsmaastrophysics/a_30_Interstellar_and_IGM_dust_Primary.doc"><IMG src="a_30_Beers_Law_out_main.jpg"></A></P>
<P><STRONG>Clifford A. Paiva_BSMRA_W5 Interstellar Shock Zone</STRONG>.&nbsp; Vortex symmetry is not possible in this zone consisting of intense electromagneto-hydrodynamic shocks; hence planetary formation is not possible, assuming incorrectly that planetary gravitational accretion physics was possible...which it is not due to outward pressure potentials and energy dissipative processes, in accordance with the Second Law of Thermodyanmics: <A href="http://smtp.antelecom.net/blogs/bsmaastrophysics/a_30_Intergalactic_Dust.pdf"><STRONG>BSMRA_</STRONG><STRONG>Intergalactic Dust.pdf</STRONG></A> </P>
<P><A href="http://smtp.antelecom.net/blogs/bsmaastrophysics/a_30_Interstellar_and_IGM_dust_Primary.doc"><IMG src="a_30_W5_Shock_out_1.jpg"></A> </P>
<P><A href="a_30_BSMRA_Arp_Objects_in_Arp_and_NGC_Sequence.pdf"><STRONG>BSMRA_Arp Objects in Arp and NGC Sequence.pdf</STRONG></A> </P>
<P><A href="http://smtp.antelecom.net/blogs/bsmaastrophysics/a_30_Clusters_and_Galaxies_in_Collision.pdf"><IMG src="a_30_NGC_1365_NO_BLACKHOLE_SOURCE.jpg"></A>&nbsp;<A href="a_30_Clusters_and_Galaxies_in_Collision.pdf"><STRONG>Clusters and Galaxies in Collision.pdf</STRONG></A> </P>
<P><STRONG><A href="http://www.google.com/search?q=Clifford+A.+Paiva+BSMRA&amp;hl=en&amp;filter=0">All BSMRA Sites</A></STRONG></P></p>
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      <em>Clifford A. Paiva @ 06:52 AM</em>
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			  <p><b>Cliff:</b> Most of the applicable equations of absorption and scattering are of course derived from James Clerk-Maxwell&#39;s field equations. Included applications to geocore geomagnetics, electromagnetic extinction, non-equilibrium radiative gas dynamics, and missile exhaust plume radiation processes. <small>(08/26/09)</small></p>
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			  <p><b>Cliff:</b> The intergalactic hydrogen and helium gas transmission fields, to say little of the inter-galactic cluster high energy fields, are excellent absorption, scattering and re-transmission media. Re-transmission is at longer wavelengths. X-ray and gamma ray sources by definition must, if the propagation of these wavelengths are observed, be at distances which do not subject such radiations to extinction processes. These sources&nbsp;should be relatively close to this solar system. <small>(08/26/09)</small></p>
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		  			<div class="comment-body"><a name=30_3></a>
			  <p><b>Cliff:</b> It is essential to remember that electromagnetic radiation emissions (including light) from a star embedded within a distant galaxy, must transit <STRONG><U><EM>multiply through interstellar media (ISM) and intergalactic medium (IGM</EM></U></STRONG>). This includes (1.) the originating&nbsp;star's ISM and IGM, and (2.) the observation galaxy's (Milky Way) IGM&nbsp;and our own interstellar medium (ISM), and of course our interplanetary dust medium (IPM). Also one should remember that the extinction processes of absorption, mutlitple-scattering and re-emission (at longer wavelengths and reddend spectral shifts, are inversely proportional to originating emission frequency. As the emission wavelength decreases (i.e. UV, x-rays and gamma rays), the extinction increases through optical scattering.&nbsp; This is of course one of the primary reasons why x-ray and gamma-ray emitters cannot be at extreme distances as the sources emissions would have undergone extinction before reaching our optics (i.e. telescopes).&nbsp;Long wave infrared (LWIR) and millimeter wavelengths (MMW)&nbsp; are more effective for transmission due to Rayleigh scattering <EM>around </EM>the interstellar dust particles; hence the use of infrared and radio telescopes for deep space optics. <small>(08/27/09)</small></p>
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     <h2 class="date-header">Saturday, 15 August 2009</h2>
      
   <div class="post"><a name=29></a>
    <h3 class="post-title">Clifford Anthony Paiva_BSMRA:  Intergalactic and BSMRA_Interstellar Electromagnetic Wave Absorption and Scattering Resulting in Wave Elongation (Reddening)</h3>
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<P><A href="http://smtp.antelecom.net/blogs/bsmaastrophysics/a_29_Galaxy_and_Star_Absorption_and_Emission_Lines.doc"><STRONG>BSMRA_</STRONG><STRONG>Galaxy and Star Absorption and Emission Lines.doc</STRONG></A><STRONG> <BR></STRONG><A href="http://www.universetoday.com/2009/02/26/intergalactic-dust-could-be-messing-up-observations/"><IMG src="a_29_IGM_ISM_Re-emission_out_1.jpg"></A> <BR><A href="http://apod.nasa.gov/apod/image/0101/ngc1410_keel_big.jpg"><IMG src="a_29_IGM_ISM_Re-emission_out_2.jpg"></A>&nbsp;<BR></P>
<P><STRONG>Clifford A. Paiva_</STRONG><A href="a_29_BSMRA_Arp_Objects_in_Arp_and_NGC_Sequence.pdf"><STRONG>BSMRA_Arp Objects in Arp and NGC Sequence.pdf</STRONG></A> </P>
<P><STRONG>Clifford A. Paiva_<A href="http://nedwww.ipac.caltech.edu/level5/Arp/Arp_contents.html">BSMRA_Halton Arp's Peculiar Galaxy Catalogue</A></STRONG></P></p>
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      <em>Clifford A. Paiva @ 14:06 PM</em>
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			  <p><b>Cliff:</b> Electromagnetic waves originating from stars and galaxies undergo absorption, multiple scattering, and re-emission (at longer wavelengths and lower frequencies) processes. When viewed through appropriate optics (telescopes, spectrometers, etc.) the absorption and emission lines are usually shifted to longer wavelengths, or "reddened". Note that this&nbsp;electromagnetic extinction&nbsp;process&nbsp;is not a function of galaxy or star displacement velocities, but rather the physical characteristics of the intergalactic and interstellar transmission fields (i.e. interstellar carbonaceous silicates and graphites). Gravitational redshifting may also be involved. Big Bang models which require a <EM>dopple</EM>r interpretation for the absorption and emission line spectral shifts are based on a <FONT face="times new roman,serif">false assumption regarding the generating function of the spectral sh</FONT>ift. <small>(08/15/09)</small></p>
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     <h2 class="date-header">Thursday, 30 April 2009</h2>
      
   <div class="post"><a name=28></a>
    <h3 class="post-title">Clifford Anthony Paiva_BSMRA:  Arp 165 NGC 2418 Vortex System, Arp 152 [Messier 87] Represents Intensity Galactic Vortex</h3>
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<P><FONT color=#3333ff><STRONG>BSM Research maintains that <A href="http://nedwww.ipac.caltech.edu/level5/Arp/Arp_contents.html">Arp 152 [M87]</A> and Arp 165 NGC 2418 represent intense galactic vortices.&nbsp; As in all vortices, mass is primarily directed to the center of the vortex.&nbsp;Curl of the velocity vector is not zero, spiral characteristics notwithstanding.</STRONG></FONT></P>
<P><A href="http://apod.nasa.gov/apod/image/0101/ngc1410_keel_big.jpg"><IMG src="a_28_Messier_87_Arp_152.jpg"></A>&nbsp;<A href="http://smtp.antelecom.net/blogs/bsmaastrophysics/a_28_Arp_165_NGC_2418_Vortex.pdf"><IMG src="a_28_Arp_165_NGC_2418.jpg"></A> </P>
<P><STRONG><A href="http://smtp.antelecom.net/blogs/bsmaastrophysics/a_28_Arp_165_NGC_2418_Vortex.pdf">Clifford A. Paiva_BSMRA:</A></STRONG> <A href="a_28_Arp_165_NGC_2418_Vortex.pdf"><STRONG>Arp 165 NGC 2418 Vortex.pdf</STRONG></A> </P></p>
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      <em>Clifford A. Paiva @ 22:26 PM</em>
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			  <p><b>Cliff:</b> In any case I am not convinced on Dr. Arp&#39;s ejection model for Arp 152; and certainly not for what he assumes are ejected quasars in near proximity of galaxy hosts. <small>(04/30/09)</small></p>
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     <h2 class="date-header">Monday, 09 February 2009</h2>
      
   <div class="post"><a name=26></a>
    <h3 class="post-title">Clifford Anthony Paiva_BSMRA:  Arp 166 [NGC 0750]; Arp 301[UGC 6204]: BSMRA_Hyrdrogen-Helium Intergalactic Gas Bridge</h3>
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<P>As is the case with most of the <A href="http://nedwww.ipac.caltech.edu/level5/Arp/Arp_contents.html"><STRONG>Arp collection</STRONG> </A>the gas bridges have been identified by BSM Research Associates.&nbsp; Also the common effects of gravitationally disturbed areas of the rotation arms are revealed.&nbsp; The nodule "spheres" are generated by acoustic compression zones within rotating sections of the outer vortex arms caused by these two collision galaxies.</P>
<P><A href="http://www.atnf.csiro.au/pasa/15_3/masci/paper/node4.html"><IMG src="a_26_Arp_301_out_1.jpg"></A> <BR><A href="http://www.atnf.csiro.au/pasa/15_3/masci/paper/node3.html"><IMG src="a_26_Arp_301_out_2.jpg"></A> <BR><A href="http://smtp.antelecom.net/blogs/bsmaastrophysics/a_26_Cliff_PRIMARY_Prime_Military__RESUME__2009.doc"><STRONG>BSMRA_Clifford Anthony Paiva RESUME 2009.doc</STRONG></A> <BR><A href="a_26_BSMRA_Arp_Objects_in_Arp_and_NGC_Sequence.pdf"><STRONG>BSMRA_Arp Objects in Arp and NGC Sequence.pdf</STRONG></A> </P>
<P><A href="http://smtp.antelecom.net/blogs/bsmaastrophysics/a_26_Arp_166_NGC_0750.doc"><IMG src="a_26_Arp_166_Disintergration.jpg"></A>&nbsp;</P>
<P><STRONG><A href="http://smtp.antelecom.net/blogs/bsmaastrophysics/a_26_Arp_166_NGC_0750.doc">Clifford A. Paiva_BSMRA</A>: </STRONG><A href="a_26_Arp_166_NGC_0750.doc"><STRONG>Arp 166 NGC 0750.doc</STRONG></A> </P>
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      <em>Clifford A. Paiva @ 03:44 AM</em>
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     <h2 class="date-header">Thursday, 22 January 2009</h2>
      
   <div class="post"><a name=25></a>
    <h3 class="post-title">Clifford Anthony Paiva_BSMRA:  Arp 299 [NGC 3690]; BSMRA_Arp 297 [NGC 5755 NGC 5754 NGC 5753 NGC 5752; BSMRA_ Intergalactic Dust Absorbtion and Re-Emission Yielding Apparent Velocity Doppler Shifts (NOT Real)</h3>
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      <p><P>&nbsp;<A href="http://smtp.antelecom.net/blogs/BSMRAMainsite/"><STRONG>BSMRA Main Site</STRONG></A></P>
<P><A href="http://smtp.antelecom.net/blogs/bsmaastrophysics/item_25.htm"><IMG src="a_25_Arp_297_Out_1.jpg"></A> <BR><A href="http://arxiv.org/PS_cache/arxiv/pdf/0908/0908.3712v1.pdf"><IMG src="a_25_Arp_297_Out_2.jpg"></A> <BR><A href="http://smtp.antelecom.net/blogs/bsmaastrophysics/a_25_Arp_297_NGC_5755.pdf"><STRONG>BSMRA_</STRONG><STRONG>Arp 297 NGC 5755.pdf</STRONG></A><STRONG> <BR></STRONG><A href="http://www.iop.org/EJ/article/1538-3881/125/4/1897/202220.web.pdf?request-id=6526cde3-62be-4e40-b5d8-258fad6f8a7a"><IMG src="a_25_Arp_299_out_1.jpg"></A> <BR><A href="http://en.wikipedia.org/wiki/Atlas_of_Peculiar_Galaxies"><IMG src="a_25_Arp_299_out_2.jpg"></A> <BR><A href="http://smtp.antelecom.net/blogs/bsmaastrophysics/a_25_Arp_298_and_Arp_299.pdf"><STRONG>BSMRA_</STRONG><STRONG>Arp 298 and Arp 299.pdf</STRONG></A> </P></p>
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      <em>Clifford A. Paiva @ 12:27 PM</em>
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			  <p><b>Cliff:</b> Arp 297 [NGC 5755/54/53/52] is a good example of intergalactic gas field absorption and re-emission at longer wavelegths and lower frequencies.  Electromagnetic gas extinction (absorption, multiple scattering, and re-emission) processes are normally misinterpreted by folks attempting to use the Hubble &#34;constant&#34; for doppler velocity applications, thus ignoring electromagnetic wave propagation physics; particularly in hopes of substantiating the existence of the Big Bang.  All galaxies within the Arp 297 system are in fact indigeneous to that galaxy matrix. <small>(01/22/09)</small></p>
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		  			<div class="comment-body"><a name=25_2></a>
			  <p><b>Cliff:</b> Arp 299 [NGC3690] is in collision. These frames reveal a gas-rich (MHI=3.3E9 Msun) optically thin(mB~27 magnitude arcsec-2),  tidal excited gas tail with a length of over 180 kpc (3.261light years). <small>(01/29/09)</small></p>
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		<p class="profile-textblock">[PLEASE USE CONTROL (+) FOR ZOOMS AND CONTROL (0) FOR NORMAL VIEW].  Large Scale Structures (Geller Shock Compression Zones) clearly reveal the presence of voids (magnetohydrodynamic rarefaction zones).  This analysis was originally implemented by Dr. Lars Lindberg Christensen, University of Copenhagen, Denmark. The zones
in the immediate areas of the shock lines are in excess of 100 million degree-C.  WITHIN the shock lines temperatures are yet to be determined.  The surrounding area temperatures are 10-20 million deg-C.  Folks interested in astrophysical heat processes from a Biblical perspective may reference: 

2Pe 3:10:
But the day of the Lord will come like a thief, in which the heavens will pass away with a roar and the elements will be destroyed with intense heat, and the earth and its works will be burned up. 

2Pe 3:12:
...looking for and hastening the coming of the day of God, because of which the heavens will be destroyed by burning, and the elements will melt with intense heat!...

Re 16:9:
Men were scorched with fierce heat; and they blasphemed the name of God who has the power over these plagues, and they did not repent so as to give Him glory. 

The last statement from Revelation 16:9 may also be connected to the global heating and solar radiance and storm (sunspot ) frequency increases, also assessed in this website (please refere to the Sections listing).

THIS SITE INCLUDES THE UNIVERSITY OF TEXAS AT EL PASO (PHYSICS DEPARTMENT) THOMAS G. BARNES AND HAROLD S. SLUSHER FILES

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		    <a href="http://smtp.antelecom.net/blogs/bsmaastrophysics/item_32.htm">
		       Clifford Anthony Paiva_BSMRA:  Single Background Frame for BSMRA_Fomalhaut Star System Used TWICE; BSMRA_Fomalhaut B; Accumulation Dust Zone Centers (DZC); HR 8799 DZCs and Not  Yet Confirmed Planets Without Assumptions Implemented 		    </a>
		  </li>
        		  <li>
		    <a href="http://smtp.antelecom.net/blogs/bsmaastrophysics/item_31.htm">
		       Clifford Anthony Paiva_BSMRA:  Stardust Mission Integrity Questions: The Isotopic Abundance of Glycine-Carbon-13 On Earth and Mission Contamination 		    </a>
		  </li>
        		  <li>
		    <a href="http://smtp.antelecom.net/blogs/bsmaastrophysics/item_30.htm">
		       Clifford Anthony Paiva_BSMRA:  Disintegration of Vortex Galaxies; So-Called "Quasars":  Normal Stars and Galaxies; Dr. Halton Arp (Max Planck Institute); Assumed Doppler Interpretation for Redshift and Application Within the BSMRA_Hubble Constant; Closed Science 		    </a>
		  </li>
        		  <li>
		    <a href="http://smtp.antelecom.net/blogs/bsmaastrophysics/item_29.htm">
		       Clifford Anthony Paiva_BSMRA:  Intergalactic and BSMRA_Interstellar Electromagnetic Wave Absorption and Scattering Resulting in Wave Elongation (Reddening) 		    </a>
		  </li>
        		  <li>
		    <a href="http://smtp.antelecom.net/blogs/bsmaastrophysics/item_28.htm">
		       Clifford Anthony Paiva_BSMRA:  Arp 165 NGC 2418 Vortex System, Arp 152 [Messier 87] Represents Intensity Galactic Vortex 		    </a>
		  </li>
        		  <li>
		    <a href="http://smtp.antelecom.net/blogs/bsmaastrophysics/item_26.htm">
		       Clifford Anthony Paiva_BSMRA:  Arp 166 [NGC 0750]; Arp 301[UGC 6204]: BSMRA_Hyrdrogen-Helium Intergalactic Gas Bridge 		    </a>
		  </li>
        		  <li>
		    <a href="http://smtp.antelecom.net/blogs/bsmaastrophysics/item_25.htm">
		       Clifford Anthony Paiva_BSMRA:  Arp 299 [NGC 3690]; BSMRA_Arp 297 [NGC 5755 NGC 5754 NGC 5753 NGC 5752; BSMRA_ Intergalactic Dust Absorbtion and Re-Emission Yielding Apparent Velocity Doppler Shifts (NOT Real) 		    </a>
		  </li>
        		  <li>
		    <a href="http://smtp.antelecom.net/blogs/bsmaastrophysics/item_23.htm">
		       Clifford Anthony Paiva_BSMRA:  Arp 290 [IC 0195-96]; BSMRA_Arp 291 [UGC 05832]; BSMRA_Arp 293 [NGC 6286-85]; BSMRA_Mass Loss  		    </a>
		  </li>
        		  <li>
		    <a href="http://smtp.antelecom.net/blogs/bsmaastrophysics/item_22.htm">
		       Clifford Anthony Paiva_BSMRA:  Arp 23; BSMRA_Arp 269; BSMRA_Arp 287; BSMRA_Arp 288 		    </a>
		  </li>
        		  <li>
		    <a href="http://smtp.antelecom.net/blogs/bsmaastrophysics/item_18.htm">
		       Clifford Anthony Paiva_BSMRA:  Spectral Redshifts: BSMRA_NGC 7320 (Arp 319); BSMRA_Arp 289 [NGC 3981]: Gas Connection Zones 		    </a>
		  </li>
        		  <li>
		    <a href="http://smtp.antelecom.net/blogs/bsmaastrophysics/item_16.htm">
		       Clifford Anthony Paiva_BSMRA:  Arp 167 [NGC 2672 +73; Arp 319 BSMRA_[Messier 65-66]; BSMRA_Arp 319 [NGC 7320] System 		    </a>
		  </li>
        		  <li>
		    <a href="http://smtp.antelecom.net/blogs/bsmaastrophysics/item_15.htm">
		       Clifford Anthony Paiva_BSMRA:  Arp 168 NGC 221; Arp 272 [NGC 6050]; BSMRA_ Arp 286 [NGC 5566] NGC 5560 NGC 5569; 		    </a>
		  </li>
        		  <li>
		    <a href="http://smtp.antelecom.net/blogs/bsmaastrophysics/item_14.htm">
		       Clifford Anthony Paiva_BSMRA:  Arp 271[NGC 5426, NGC 5427]; BSMRA_Arp 87 [NGC 3808; NGC 3808] A Physically Connected Through Vortex Center Region 		    </a>
		  </li>
        		  <li>
		    <a href="http://smtp.antelecom.net/blogs/bsmaastrophysics/item_11.htm">
		       Clifford Anthony Paiva_BSMRA:  The Thomas G. Barnes and Harold S. Slusher Physics Files and Publications 		    </a>
		  </li>
        		  <li>
		    <a href="http://smtp.antelecom.net/blogs/bsmaastrophysics/item_10.htm">
		       Clifford Anthony Paiva_BSMRA:  Arp 281 [NGC 4631 and 4627] In Violent Collision; BSMRA_ARP 269 [NGC 4485 and NGC 4490]  With  Gas Bridge Connection And In Intergalactic Collision 		    </a>
		  </li>
        		  <li>
		    <a href="http://smtp.antelecom.net/blogs/bsmaastrophysics/item_5.htm">
		       Clifford Anthony Paiva_BSMRA:  Large Scale Structures; BSMRA_Super Cluster Vortices Concentration; BSMRA_Standing Wave Shock Zones; BSMRA_Super Cluster Collision; BSMRA_ Inter-Galactic Cluster 100 Million Degree X and BSMRA_Gamma Ray Temperatures 		    </a>
		  </li>
        		  <li>
		    <a href="http://smtp.antelecom.net/blogs/bsmaastrophysics/item_3.htm">
		       Clifford Anthony Paiva _BSMRA:  Galaxy Disintegration Processes; Geller Lines; Arp 286; Markarian 205 CONNECTION; Arp 282, NGC 0169; Arp 283; NGC 2798; Arp 314; Stephan's Quintet NGC 7320 CONNECTION; galactic Gas Diffusion; NGC 4319; Arp 290;Electromagnetic Propagation Extinction; Galaxy Mass-Loss; BSMRA_Galaxy and BSMRA_Cluster Collisions 		    </a>
		  </li>
        		  <li>
		    <a href="http://smtp.antelecom.net/blogs/bsmaastrophysics/item_2.htm">
		       Clifford Anthony Paiva_ BSMRA:  Galaxy Disintegration Processes; Electromagnetic Propagation Extinction; BSMRA_Geller LInes; BSMRA_ Arp 278; BSMRA_Arp 284;  Arp 286; NGC 5566; NGC 4319 Connecton; BSMRA_Arp 27, NGC 7578; Arp 26; M 101; Arp 3; Arp 41; NGC 1232; Arp 85, M 51CONNECTION; Arp 29, NGC 6946; Arp 27; Arp 93; Arp 84; Arp 112, BSMRA_NGC 7805; Arp 278, BSMRA_NGC 7253; 		    </a>
		  </li>
        
    </ul>
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