Hostname: page-component-586b7cd67f-dlnhk Total loading time: 0 Render date: 2024-11-30T01:38:51.250Z Has data issue: false hasContentIssue false
  • English
  • Français

Color Distribution of Faint Galaxies and Quasi-Stellar Objects

Published online by Cambridge University Press:  04 August 2017

Richard G. Kron
Richard G. Kron*
Affiliation:
Yerkes Observatory, The University of Chicago

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.

The apparent colors in a flux-complete sample of galaxies depend on the redshifts and the spectral types in the sample. These in turn depend on both luminosity evolution and evolution of the shapes of the spectra. Thus in principle a great deal about the evolution of galaxies can be learned from complete multicolor surveys, especially now that large samples can be routinely generated by automatic machine measurement. The following will review what has been learned from recent work.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 104: Early Evolution of the Universe and Its Present Structure , 1983 , pp. 95 - 99
Copyright
Copyright © Reidel 1983 

References

Aaronson, M.: 1977, , Harvard University.Google Scholar
Arp, H., and Surdej, J.: 1982, A.&A. 109, pp. 101–106.Google Scholar
Bruzual, A.G.: 1981, , University of Calif., Berkeley.Google Scholar
Butchins, S.A.: 1981, A.&A. 97, pp. 407–409.Google Scholar
Butchins, S.A.: 1982, preprint.Google Scholar
Couch, W.J.: 1981, , Australian National University.Google Scholar
Ellis, R.S., and Allen, D.A.: 1982, AAO preprint No. 167.Google Scholar
Formiggini, L., Zitelli, V., Bonoli, F., and Braccesi, A.: 1980, A.&A Suppl. 39, pp. 129–132.Google Scholar
Grasdalen, G.L.: 1980, in IAU Symp. No. 92, eds. Abell, G.O. and Peebles, P.J.E. (Dordrecht: Reidel), pp. 269–276.Google Scholar
Harris, W.E., and Smith, M.G.: 1981, A.J. 86, pp. 90–97.Google Scholar
Karachentsev, I.D.: 1980, Sov. Astron. Lett. 6, pp. 1–2.Google Scholar
Koo, D.C.: 1981, , University of Calif., Berkeley.Google Scholar
Koo, D.C.: 1983, this volume, p. 105.Google Scholar
Koo, D.C., and Kron, R.G.: 1982, A.&A. 105, pp. 107–119.Google Scholar
Kron, R.G., and Chiu, L.-T.G.: 1981, P.A.S.P. 93, pp. 397–404.Google Scholar
Lebofsky, M.J.: 1981, Astrophys. J. (Lett.) 245, pp. L59–L62.CrossRefGoogle Scholar
Lilly, S.J., and Longair, M.S.: 1982, Mon. Not. Roy. Ast. Soc. 199, pp. 1053–1068.Google Scholar
Notni, P.: 1980, Astron. Nachr. 301, pp. 51–67.CrossRefGoogle Scholar
Pence, W.: 1976, Astrophys. J. 203, pp. 39–51.Google Scholar
Phillips, S., Fong, R., and Shanks, T.: 1981, Mon. Not. Roy. Ast. Soc. 194, pp. 49–62.Google Scholar
Puschell, J.J., Owen, F.N., and Laing, R.: 1982, Astrophys. J. (Lett.) 257, pp. L57–L61.Google Scholar
Richer, H.B., and Olsen, B.I.: 1980, P.A.S.P. 92, pp. 573–575.Google Scholar
Spinrad, H.: 1982, P.A.S.P. 94, pp. 397–403.CrossRefGoogle Scholar
Usher, P.D., and Mitchell, K.J.: 1982, Astrophys. J. Suppl. 49, pp. 27–52.Google Scholar
Valdes, F.: 1982, in S.P.I.E. Instrumentation in Astronomy IV, 331, March 1982, Tucson, ed. Crawford, D.L. Google Scholar