Hostname: page-component-848d4c4894-sjtt6 Total loading time: 0 Render date: 2024-06-22T06:25:10.698Z Has data issue: false hasContentIssue false

Luminosity Function and Spatial Distribution of Nearby Galaxies

Published online by Cambridge University Press:  26 July 2016

K.-H. Schmidt
Affiliation:
Astrophysikalisches Institut, An der Sternwarte 16, Potsdam, Germany
T. Boller
Affiliation:
Max-Planck-Institut für Extraterrestrische Physik, Karl-Schwarzschild-Strasse 2, Garching, Germany

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 investigation of environmental effects is a topic of high priority in current extragalactic research. In this connection, the study of neighbouring galaxies will result in characteristic properties of a low-density sample of extragalactic systems which may be used for comparison with other samples, with clusters of galaxies, for instance. The advantage of nearby galaxies is that they allow us to obtain an almost complete sample down to low-luminous objects because of their small distances.

Type
Part Twelve: Properties of Nearby Galaxies
Copyright
Copyright © Kluwer 1994 

References

Busarello, G., Longo, G. and Feoli, A., 1993. Astron. Astrophys., in press.Google Scholar
de Vaucouleurs, G., 1953. Astron. J., 58, 30.CrossRefGoogle Scholar
Kraan-Korteweg, R.C. and Tammann, G.A., 1979. Astron. Nachr., 300, 181.Google Scholar
Mineva, V.A., 1988. Astron. Zh., 65, 702.Google Scholar
Sandage, A., Binggeli, B. and Tammann, G.A., 1985. Astron. J., 90, 1759.Google Scholar
Schechter, P.L., 1976. Astrophys. J., 203, 297.Google Scholar
Schmidt, K.-H. and Boller, T., 1992a. Astron. Nachr., 313 189.Google Scholar
Schmidt, K.-H. and Boller, T., 1992b. Astron. Nachr., 313, 329.Google Scholar
Schmidt, K.-H., Priebe, A. and Boller, T., 1993. Astron. Nachr., in press.Google Scholar
Tully, R.B., 1988. Astron. J., 96, 73.Google Scholar
van den Bergh, S., 1992. Astron. Astrophys., 264, 75.Google Scholar