
Secular Evolution of Galaxies
Cambridge University Press
Published on 2. September 2013
Book
Hardback
650 pages
978-1-107-03527-0 (ISBN)
Description
The formation and evolution of galaxies is one of the most important topics in astrophysics. Secular evolution refers to the relatively slow dynamical evolution due to internal processes induced by a galaxy's spiral arms, bars, galactic winds, black holes and dark matter haloes. It plays an important role in the evolution of spiral galaxies with major consequences for galactic bulges, the transfer of angular momentum, and the distribution of a galaxy's constituent stars, gas and dust. This internal evolution is key to understanding cosmological models of galaxy formation and evolution. Based on the twenty-third Winter School of the Canary Islands Institute of Astrophysics, this volume presents reviews from nine experts on the observational and theoretical research into secular processes, and what these processes can tell us about the structure and formation of galaxies. The volume provides a grounding for graduate students and researchers working on galactic dynamics and galaxy evolution.
More details
Series
Language
English
Place of publication
Cambridge
United Kingdom
Target group
Professional and scholarly
Illustrations
306 Halftones, unspecified
Dimensions
Height: 260 mm
Width: 184 mm
Thickness: 34 mm
Weight
1270 gr
ISBN-13
978-1-107-03527-0 (9781107035270)
Copyright in bibliographic data and cover images is held by Nielsen Book Services Limited or by the publishers or by their respective licensors: all rights reserved.
Schweitzer Classification
Other editions
Additional editions

Jesus Falcon-Barroso | Johan H. Knapen
Secular Evolution of Galaxies
E-Book
09/2013
1st Edition
Cambridge University Press
€79.99
Available for download
Persons
Dr Jesus Falcon-Barroso is Head of the Research Group on 'Traces of Galaxy Formation' at the Instituto de Astrofisica de Canarias, Tenerife. His main research areas include the development of stellar population models, unraveling the nature of bars and bulges, and the formation and evolution of dwarf elliptical galaxies. Dr Johan H. Knapen is Head of the Research Division at Instituto de Astrofisica de Canarias, Tenerife, and a visiting professor at the University of Hertfordshire. He is an observational astronomer studying the structure, dynamics and evolution of spiral galaxies.
Editor
Instituto de Astrofisica de Canarias, Tenerife
Instituto de Astrofisica de Canarias, Tenerife
Content
Preface; 1. Secular evolution in disk galaxies John Kormendy; 2. Galaxy morphology Ronald J. Buta; 3. Dynamics of secular evolution James Binney; 4. Bars and secular evolution in disk galaxies: theoretical input E. Athanassoula; 5. Stellar populations Reynier F. Peletier; 6. Star formation rate indicators Daniela Calzetti; 7. The evolving interstellar medium Jacqueline van Gorkom; 8. Evolution of star formation and gas Nick Z. Scoville; 9. Cosmological evolution of galaxies Isaac Shlosman.