Hostname: page-component-745bb68f8f-d8cs5 Total loading time: 0 Render date: 2025-01-31T12:11:57.645Z Has data issue: false hasContentIssue false
  • English
  • Français

Ejection Phenomena in Galaxies and QSOs: Are We Going Far Enough?

Published online by Cambridge University Press:  12 April 2016

G. Burbidge
G. Burbidge*
Affiliation:
University of California, San Diego, Center for Astrophysics & Space Sciences and Department of Physics, La Jolla, CA 92093-0424, U.S.A.

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

I summarize the observational evidence which suggests: (1) that many of the compact radio sources associated with QSOs and related objects have been ejected from active galaxies so that their redshifts are not measures of their distances, and (2), that the energy emitted by compact sources is not gravitational in origin, but arises through creation processes in regions of galaxies with very strong gravitational fields.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 164: Radio Emission from Galactic and Extragalactic Compact Sources , 1998 , pp. 33 - 34
Copyright
Copyright © Astronomical Society of the Pacific 1998

References

Arp, H.C. 1987. Quasars, Redshifts & Controversies (Berkeley: Interstellar Media).Google Scholar
Burbidge, E.M. 1995. A&A, 298, Ll–4.Google Scholar
Burbidge, E.M. 1997. ApJ, 484, L99–101.Google Scholar
Burbidge, G. 1996. A&A, 309, 9–22.Google Scholar
Burbidge, G., Hoyle, F. & Schneider, P. 1997. A&A, 320, 8–12.Google Scholar
Hoyle, F. & Burbidge, G. 1996. A&A, 309, 335–344.Google Scholar
Hoyle, F., Burbidge, G., & Narlikar, J.V. 1993. ApJ, 410, 437–457.Google Scholar
Hoyle, F., Burbidge, G., & Narlikar, J.V. 1994a. MNRAS, 267, 1007–1019.Google Scholar
Hoyle, F., Burbidge, G., & Narlikar, J.V. 1994b. A&A, 289, 729–739.Google Scholar
Hoyle, F., Burbidge, G., & Narlikar, J.V. 1995. Proc. Roy. Soc. (London) A, 448, 191–212.Google Scholar