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Fundamental Observational Problems

Published online by Cambridge University Press:  25 May 2016

H. Arp
H. Arp*
Affiliation:
Max-Planck-Institut für Astrophysik, D-85740 Garching, Germany

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Almost all of cosmology and extragalactic astronomy are built on the assumption that redshifts are caused by recession velocities and hence measure distances. Evidence has been accumulating since 1966, however, that high redshift quasars and other active objects violate this assumption and are associated with nearby, relatively low redshift galaxies (For recent reviews see Arp 1987; 1992a, 1994a,b and the present conference).

Type
Part I: Invited Reviews
Information
Symposium - International Astronomical Union , Volume 168: Examining the Big Bang and the Diffuse Background Radiations , 1996 , pp. 401 - 406
Copyright
Copyright © Kluwer 1996 

References

Arp, H. 1986, Astr. Astrophysics 156, 207.Google Scholar
Arp, H. 1987, “Quasars, Redshifts and Controversies” Interstellar Media, Berkeley.Google Scholar
Arp, H. 1992a, IAU Highlights of Astronomy 9, 43.Google Scholar
Arp, H. 1992b, Phys. Lett. A 168, 6.Google Scholar
Arp, H. 1993, Progress in New Cosmologies, Proceedings of XIII Cracow School of Cosmology, Plenum Press, p2.CrossRefGoogle Scholar
Arp, H. 1994a, Frontiers of Fundamental Physics, Proceedings of the Olympia Conference, ed. Selleri, F. and Barone, M., Plenum Publ. Corp. Google Scholar
Arp, H. 1994b, Ap.J. 430, 74.CrossRefGoogle Scholar
Böhringer, H., Briel, U.G., Schwarz, R.A., Voges, W., Hartner, G. and Trümper, J. 1994, Nature 368, 828.Google Scholar
Napier, W.M. and Guthrie, B.N.G. 1993, Progress in New Cosmologies, Proceedings of XIII th Cracow School of Cosmology, Plenum Press, p.29.CrossRefGoogle Scholar
Narlikar, J.V. and Arp, H.C. 1993, Ap.J. 405, 51.Google Scholar
Pietsch, W., Vogler, A., Kahabka, P., Jain, A. and Klein, U. 1994, Astr. Astrophys. 284, 386.Google Scholar