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A phenomenological approach to the evolution of galaxies

Published online by Cambridge University Press:  17 July 2013

Simon J. Lilly ,
Yingjie Peng ,
Marcella Carollo  and
Alvio Renzini
Simon J. Lilly
Affiliation:
Institute of Astronomy, ETH Zurich, 8093 Zurich, Switzerland
Yingjie Peng
Affiliation:
Institute of Astronomy, ETH Zurich, 8093 Zurich, Switzerland
Marcella Carollo
Affiliation:
Institute of Astronomy, ETH Zurich, 8093 Zurich, Switzerland
Alvio Renzini
Affiliation:
INAF Osservatorio Astronomico di Padova, vicolo dell'Osservatorio 5, I-35122 Padova, Italy, and Department of Physics and Astronomy Galileo Galilei, Universita degli Studi di Padova, via Marzolo 8, I-35131Padova, Italy
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Abstract

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Increasingly good statistical data on the galaxy population at high and low redshift enable the development of new phenomenological approaches to galaxy evolution based on application of the simplest continuity equations. This has given new insights into the different ways in which star-formation in galaxies is quenched, the role of merging in the population, and in to the control of star-formation in star-forming galaxies and the links with chemical evolution. The continuity approach provides a self-consistent view of the evolving population and exposes linkages between different aspects of galaxy evolution.

Keywords

Galaxy evolutionstar-formation ratechemical evolution
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S295: The intriguing life of massive galaxies , August 2012 , pp. 141 - 150
Copyright
Copyright © International Astronomical Union 2013 

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