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Measuring the Evolution of the Mass-to-Light Ratio from z = 0 to z = 0.6 from the Fundamental Plane

Published online by Cambridge University Press:  25 May 2016

Marijn Franx ,
Pieter van Dokkum ,
Dan Kelson ,
Garth Illingworth  and
Dan Fabricant
Marijn Franx
Affiliation:
Kapteyn Astronomical Institute, Groningen, The Netherlands
Pieter van Dokkum
Affiliation:
Kapteyn Astronomical Institute, Groningen, The Netherlands
Dan Kelson
Affiliation:
University of California, Santa Cruz, USA
Garth Illingworth
Affiliation:
University of California, Santa Cruz, USA
Dan Fabricant
Affiliation:
Center for Astrophysics, Cambridge, USA

Abstract

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Galaxy evolution is probably a complex process. Mergers, infall, and starbursts may change galaxy properties systematically with time. As a result, the interpretation of the luminosity function is ambiguous, and information on the mass evolution of galaxies is needed. Such information can be retrieved from the evolution of the Tully-Fisher relation, Faber-Jackson relation, or the Fundamental Plane with redshift.

Type
Deep Fields & Evolution
Information
Symposium - International Astronomical Union , Volume 186: Galaxy Interactions at High and Low Redshift , 1999 , pp. 447 - 457
Copyright
Copyright © Kluwer 1999 

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