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The rapidly expanding field of galaxy formation lies at the interface between astronomy, particle physics, and cosmology. Covering diverse topics from these disciplines, all of which are needed to understand how galaxies form and evolve, this book is ideal for researchers entering the field. Individual chapters explore the evolution of the Universe as a whole and its particle and radiation content; linear and nonlinear growth of cosmic structure; processes affecting the gaseous and dark matter components of galaxies and their stellar populations; the formation of spiral and elliptical galaxies; central supermassive black holes and the activity associated with them; galaxy interactions; and the intergalactic medium. Emphasizing both observational and theoretical aspects, this book provides a coherent introduction for astronomers, cosmologists, and astroparticle physicists to the broad range of science underlying the formation and evolution of galaxies.
- Sales Rank: #906447 in Books
- Published on: 2010-06-28
- Original language: English
- Number of items: 1
- Dimensions: 9.72" h x 1.57" w x 6.85" l, 3.90 pounds
- Binding: Hardcover
- 840 pages
Review
"Unraveling the origin and growth of cosmic structures, from the simplicity of the Big Bang to the complexity of the modern Universe, is an unparalleled achievement of modern science. Written by renowned world experts, this book presents a clear, systematic and comprehensive exposition of the physics and mathematics underlying these breathtaking advances. It is compulsory reading not only for those aspiring to contribute to our growing understanding of the cosmos, but for all those who appreciate the beauty and power of contemporary physical science." - Carlos S. Frenk, Ogden Professor of Fundamental Physics, Director, Institute for Computational Cosmology, Durham University
"...a comprehensive text on the modern subject of galaxy formation and evolution. The book is fully self-contained, covering the basic theory in depth, and including the essential background material on observations and the relevant theory from extragalactic astronomy, stellar astrophysics, and cosmology. It will serve as an indispensable reference for students and researchers alike, and is destined to become a classic in this field." - Robert C. Kennicutt, Jr., Plumian Professor of Astronomy and Experimental Philosophy, Director, Institute of Astronomy, University of Cambridge
"Every topic is extremely well referenced and current ... This book is likely to be an essential reference for any galaxy-formation-research student or professor. In the coming years I can see myself dipping into this treasure trove on a very regular basis." Shaun Cole, The Observatory
"...an ideal introduction for anyone with a minimal background in astrophysics who wishes to enter the field of large-scale structure formation. It is well suited for use in a general astrophysics course for senior- undergraduate and graduate students and is also an excellent reference source for more advanced courses on specific topics in astrophysics. The authors are leading theoretical astrophysicists who have made major contributions to galaxy formation theory. Their text provides a comprehensive review of relevant topics, ranging from the growth of the first density fluctuations to the evolution of the stellar populations in galaxies. It is a timely update of similar but now more dated texts...." Physics Today
About the Author
Houjun Mo is Professor of Astrophysics at the University of Massachusetts. He is known for his work on the formation and clustering of galaxies and their dark matter halos.
Frank van den Bosch is Associate Professor at the University of Utah, and is known for his studies of the formation, dynamics, and clustering of galaxies.
Simon White is Director at the Max Planck Institute for Astrophysics in Garching. He is one of the originators of the modern theory of galaxy formation and has received numerous international prizes and honors.
Most helpful customer reviews
9 of 9 people found the following review helpful.
The definitive work
By Revanchist
Although there are several excellent textbooks in the area, I firmly believe that this one will become the standard reference in the area. The breadth of the topics covered alone would make it shoot up to the ranks of the top, and when one factors in all the detailed calculations and results that are presented to make the book wholly self-contained, it is easy to see why this book deserves to become the definitive work in galaxy formation and evolution.
The first two chapters present a general theoretical and observational overview of the subject, but the real fun begins from the third chapter. The three authors have chosen to follow the cosmological timeline, and hence chapters 3 and 4 deal with cosmology. Chapter 3 which lays the background for cosmology is brilliant, and could serve as a self-contained monograph on the subject. The next chapter which treats cosmological perturbations is equally noteworthy for its treatment, both Newtonian and relativistic, of small perturbations. Chapter 5 leads up to the episode of gravitational collapse and the subsequent consequences. At this point, several techniques used in probing the cosmos such as correlation functions, gravitational lensing, etc are presented in Chapter 6. Chapters 7 and 8 focus on halo formation, the former on dark matter and the latter on gas. Both these chapters cover some very important topics such as the Press-Schechter formalism, radiative cooling, etc. Chapter 8 also features a nice, though compact, discussion of fluid dynamics and instabilities. Chapters 9 and 10 are concerned with the formation and evolution of stars. Topics such as the star formation efficiency, the IMF, population synthesis, etc were presented in a clear and detailed manner. Chapters 11, 12 and 13 are primarily concerned with the types of galaxies and the interactions that can occur between galaxies. The formation of disk and elliptic galaxies, sections on dynamical friction and disk instabilities are some of the best features in these chapters. Chapter 14 deals with AGNs and the properties of active galaxies. The statistics and distribution of galaxies are looked at in Chapter 15. The last chapter is on the IGM and is one of the best chapters in the book; it could again serve as a monograph on the subject by itself.
There are several cutting edge topics presented through all the chapters. For instance, Chapter 9 features an entire section on Pop III stars, which is an active area of research currently. In a book this long and packed with detail, there are bound to be a few aspects of the book which one may find fault with. I felt that some topics such as gravitational lensing and the Press-Schechter formalism could have been covered in a more lucid manner, since some of the derivations and the discussion tended to get unnecessarily complicated at times.
These are only a few minor glitches in an outstanding work. A truly remarkable book and (one hopes) is destined to become the Bible of galaxy formation and evolution.
4 of 4 people found the following review helpful.
The grad student's helper
By Tim
Are you a graduate student in astronomy? Do you own this book? If not, go buy it **right now**. This book digests thirty years of literature in astronomy, touching such diverse subjects as nucleosynthesis to the ten-fold decrease in star formation since z~1 and QSO absorption spectra to SPH simulations. It will be a useful reference text in all of your classes. Is it intended for the arm-chair astronomer? Definitely not. But it is readable, assuming you have a fundamental understanding of astrophysical processes. And it will save any grad student a great many hours of reading through ADS.
1 of 1 people found the following review helpful.
Bible of Cosmology and Galaxy Evolution
By lee
This is written at the graduate / research level. It provides a detailed explanation of both cosmological and galaxy evolution topics. I particularly enjoyed the discussion of cosmological perturbations, inflation and the CMB. I have many times used it as a starting point when investigating a new topic in my research field.
It is extremely densely written, but all the information and equations are there. It may be dense but it is well explained, provided you take the time to read it. This is a great companion text to Binney and Tremaine's "Galactic Dynamics".
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