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The Effect of Galaxy Mergers in the Local Galaxy Population

Published online by Cambridge University Press:  01 August 2006

Leda Sampson  and
Neil Trentham
Leda Sampson
Affiliation:
Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge, CB3 0HA, UK
Neil Trentham
Affiliation:
Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge, CB3 0HA, UK
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The luminosity function (LF) is one of the most fundamental quantities to be observed in Astronomy. It is determined by the combined effects of the various physical phenomena that drive galaxy formation and evolution, therefore it is a very useful tool to constrain cosmological models.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S235: Galaxy Evolution Across the Hubble Time , August 2006 , pp. 241
Copyright
Copyright © International Astronomical Union 2007

References

Abazajian, K., 2004, AJ, 128, 502.Google Scholar
Blanton, M. R. 2003, ApJ, 592, 819.CrossRefGoogle Scholar
Colless, M., 2001, MNRAS, 328, 1039.CrossRefGoogle Scholar
Driver, S. & de Propis, R., 2003, Ap&SS, 285, 175.Google Scholar
Karachentsev, I. D., 2004, AJ, 127, 2031.Google Scholar
Trentham, N., Sampson, L. & Banerji, M., 2005, MNRAS, 357, 783.Google Scholar
Trentham, N. & Tully, R. B., 1992, MNRAS, 335, 712.CrossRefGoogle Scholar
Tully, R. B., 1988, ngc book.Google Scholar