Clifford Anthony Paiva_BSMRA: Spectral Redshifts: BSMRA_NGC 7320 (Arp 319); BSMRA_Arp 289 [NGC 3981]: Gas Connection Zones
Messier 65-66; Arp 319 NGC 7320 System and Doppler Velocity Interpretations
Doppler interpretations for the spectral shifts of the Stephan's Quintet System (Arp 319; NGC 7320) of galaxies may be correct only if the collective system has been in existence for a brief duration. Such a short period may be sufficient to prevent velocity-breakup. Far more challenging is the problem of electromagnetic wave propagation through the http://images.google.com/imgres?imgurl=http://pagesperso-orange.fr/lempel/hhn4319a.jpg&imgrefurl=http://pagesperso-orange.fr/lempel/red_shift_NGC_4319_uk.htm&usg=__253f5n8CaLVICzr9SKtSO8VTXTg=&h=444&w=444&sz=116&hl=en&start=4&tbnid=52Y7-uoKmretIM:&tbnh=127&tbnw=127&prev=/images%3Fq%3Dredshift%2Bcontroversy%2Barp%26gbv%3D2%26hl%3Den%26client%3Dfirefox-a%26rls%3Dorg.mozilla:en-US:officialhydrogen-helium intergalactic gas connection zones. These zones generate electromagnetic absorption, scattering and re-emission at longer wavelengths (reddening) of radiation emission from the galaxies. Spectral shifts through these transmission zones would certainly occur and not be associated with velocity dopplers: (la-lb)/la) = n/c (la-lb) represents EM propagation before and after exiting the transmission field gas zone; n/c represents the EM exiting frequency to the velocity of Integrated Field System (IFS) propagation commonly referred to as the speed of "light". It should be remember that "light" is a very restricted electromagnetic bandpass which is observed at ..398-.789 microns (millionth of a meter). In any case it is not possible for electromagnetic radiation to propagate through interstellar and intergalactic space without undergoing dissipative and extinction processes. And of course gravitation-reddening must be considered for the Stephan Quintet system.


BSMRA_Halton Arp Peculiar Galaxy Catalogue
Clifford Anthony Paiva RESUME 2010.doc
Astrogeophysics: T.G. Barnes, D.Sc.; H.S. Slusher Ph.D., D.Sc.; C.A. Paiva, M.S.




