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Galaxy Luminosity Function based on the Press-Schechter Theory

Published online by Cambridge University Press:  25 May 2016

H. Yoshida ,
M. Umemura  and
Y. Yoshii
H. Yoshida
Affiliation:
Fukushima Medical College, Fukushima City, Japan
M. Umemura
Affiliation:
Univ. of Tsukuba, Tsukuba, Japan
Y. Yoshii
Affiliation:
Univ. of Tokyo, Mitaka, Japan

Extract

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We investigate the cosmological model dependence of galaxy luminosity function (GLF) obtained by the Press–Schechter (PS) prescription. We consider the power–law spectra as well as a CDM spectrum for primordial density fluctuations, assuming a variety of cosmological models. We do not consider any galaxy luminosity (chemical) evolution in this report.

Type
IV. Structure Formation and Dark Matter
Information
Symposium - International Astronomical Union , Volume 183: Cosmological Parameters and the Evolution of the Universe , 1999 , pp. 275
Copyright
Copyright © Kluwer 1999