Hostname: page-component-cc8bf7c57-ksm4s Total loading time: 0 Render date: 2024-12-12T07:50:10.110Z Has data issue: false hasContentIssue false
  • English
  • Français

A Spectroscopic Search for Galaxies Associated with Quasi-Stellar Objects∗

Published online by Cambridge University Press:  14 August 2015

Joseph S. Miller ,
Howard B. French  and
Steven A. Hawley
Joseph S. Miller
Affiliation:
Lick Observatory, Board of Studies in Astronomy and Astrophysics, University of California, Santa Cruz
Howard B. French
Affiliation:
Lick Observatory, Board of Studies in Astronomy and Astrophysics, University of California, Santa Cruz
Steven A. Hawley
Affiliation:
Lick Observatory, Board of Studies in Astronomy and Astrophysics, University of California, Santa Cruz

Extract

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.

It is generally assumed that quasi-stellar objects represent phenomena taking place in galaxies. There are at least three lines of reasoning that lead to this viewpoint. First, there appears to be a continuity of properties extending from Seyfert galaxies and N systems to QSOs with the differences between the various groups principally a question of the contrast between the luminous central object and its surrounding galaxy. Since Seyfert galaxies and N systems are definitely in galaxies, it is concluded that QSOs must also be in galaxies which are not directly visible because of the high luminosity of the central object. A second argument is based on the result that QSOs do not appear to differ dramatically in abundances of elements from those which are typical of normal galaxies. With the prevailing view that virtually all the elements heavier than helium originated as a result of stellar processes, it would be concluded that QSOs must be associated with galaxies of stars that produced the heavier elements. A third, rather indirect argument is based on the results of Stockton (see his paper in this volume) and others that QSOs are often found in groups of galaxies and therefore are likely to be located in galaxies themselves (guilt by association). But the fact is that direct evidence that QSOs are in galaxies is sadly lacking.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 92: Objects of High Redshift , 1980 , pp. 83 - 87
Copyright
Copyright © Reidel 1980 

References

Miller, J. S. 1980, Pub. A. S. P. , in preparation.Google Scholar
Miller, J. S., French, H. B., and Hawley, S. A. 1978a, in Pittsburgh Conf. BL Lac Ob. , p. 176.Google Scholar
Miller, J. S., French, H. F., and Hawley, S. A. 1978b, Ap. J. (Letters) 219, L85.CrossRefGoogle Scholar
Miller, J. S., and Hawley, S. A. 1977, Ap. J. (Letters) , 212, L47.CrossRefGoogle Scholar
Miller, J. S., Robinson, L. B., and Wampler, E. J. 1976, in Advances in Electronics and Electron Physics (New York: Academic Press) Vol. 408, p. 693.Google Scholar
Richstone, D. O., and Oke, J. B. 1977, Ap. J. , 213, 8.CrossRefGoogle Scholar
Sandage, A. 1972, Ap. J. , 173, 485.Google Scholar
Wampler, E. J., Robinson, L. B., and Burbidge, E. M. and Baldwin, J. A. 1975, Ap. J. (Letters) , 198, L49.Google Scholar