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Cosmological evolution of galaxies

Published online by Cambridge University Press:  05 September 2013

Isaac Shlosman
Affiliation:
University of Kentucky
Jesús Falcón-Barroso
Affiliation:
Instituto de Astrofísica de Canarias, Tenerife
Johan H. Knapen
Affiliation:
Instituto de Astrofísica de Canarias, Tenerife
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Summary

Abstract

I review the subject of the cosmological evolution of galaxies, including different aspects of growth in disk galaxies, by focussing on the angular momentum problem, mergers, and their by-products. I discuss the alternative to merger-driven growth – cold accretion and related issues. In the follow-up, I review possible feedback mechanisms and their role in galaxy evolution. Special attention is paid to high-redshift galaxies and their properties. In the next step, I discuss a number of processes, gas- and stellar-dynamical, within the central kiloparsec of disk galaxies, and their effect on the larger spatial scales, as well as on the formation and fuelling of the seed black holes in galactic centres at high redshifts.

Introduction: the paradigm of galaxy evolution

The aim of these lectures is to review the main aspects of secular galaxy evolution, i.e., galaxy evolution on cosmological scales. Two issues stand out in this attempt. First, the subject is immense and cannot be covered within the scope of this chapter. And second, one cannot ignore the fact that galaxy evolution is part of the overall evolution in the Universe – from the largest spatial scales ruled by dark matter (DM) to the smallest ones taken over by dissipative baryons that can form stars and grow supermassive black holes (SMBHs). In other words, the process of galaxy formation can be influenced strongly by a huge range of spatial scales.

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Publisher: Cambridge University Press
Print publication year: 2013

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To send content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about sending content to Dropbox.

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Send book to Google Drive

To send content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about sending content to Google Drive.

Available formats
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