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Introduction to Galaxy Formation and Evolution: From Primordial Gas to Present-Day Galaxies [Kietas viršelis]

(Universitą di Bologna), (Universitą di Bologna), (Rijksuniversiteit Groningen, The Netherlands)
  • Formatas: Hardback, 582 pages, aukštis x plotis x storis: 252x192x30 mm, weight: 1410 g, 3 Halftones, black and white; 242 Line drawings, black and white
  • Išleidimo metai: 17-Oct-2019
  • Leidėjas: Cambridge University Press
  • ISBN-10: 1107134765
  • ISBN-13: 9781107134768
Kitos knygos pagal šią temą:
  • Formatas: Hardback, 582 pages, aukštis x plotis x storis: 252x192x30 mm, weight: 1410 g, 3 Halftones, black and white; 242 Line drawings, black and white
  • Išleidimo metai: 17-Oct-2019
  • Leidėjas: Cambridge University Press
  • ISBN-10: 1107134765
  • ISBN-13: 9781107134768
Kitos knygos pagal šią temą:
The Universe is filled with beautiful galaxies, made of stars, gas and dark matter, that formed during nearly fourteen billion years since the Big Bang. This advanced textbook, bridging the gap between introductory and specialized texts, reveals the complex physical processes of galaxy formation and evolution within a cosmological context.

Present-day elliptical, spiral and irregular galaxies are large systems made of stars, gas and dark matter. Their properties result from a variety of physical processes that have occurred during the nearly fourteen billion years since the Big Bang. This comprehensive textbook, which bridges the gap between introductory and specialized texts, explains the key physical processes of galaxy formation, from the cosmological recombination of primordial gas to the evolution of the different galaxies that we observe in the Universe today. In a logical sequence, the book introduces cosmology, illustrates the properties of galaxies in the present-day Universe, then explains the physical processes behind galaxy formation in the cosmological context, taking into account the most recent developments in this field. The text ends on how to find distant galaxies with multi-wavelength observations, and how to extract the physical and evolutionary properties based on imaging and spectroscopic data.

Recenzijos

'An impressive achievement which presents a detailed account of the remarkable progress in our understanding of how galaxies formed and evolved over the past 13 billion years. The authors have brought together the latest theoretical and observational developments in this fast-paced subject carefully explaining with helpful illustrations the underlying physical concepts.' Richard Ellis, University College London 'This is an admirable introduction to the formation of the galaxies, a key aspect of modern cosmology, and blends fundamental aspects of astrophysics with recent observational constraints.' Joseph Silk, Institut d'Astrophysique de Paris 'With a broad sweep of physics and a wide canvas, this book is pitched at the level of master's and graduate students. From diffuse gas through dark matter haloes to galaxies today, this is an excellent text to learn the narrative of modern theories of galaxy formation.' Wyn Evans, University of Cambridge 'Our picture of galaxy formation and evolution, though still tentative and incomplete, is one of the major scientific achievements of the past half century. But seeing this picture in its full glory has mostly been the privilege of professional researchers in the field. Cimatti, Fraternali, and Nipoti have aimed to open the view to astrophysics students at the master's level, and they have succeeded brilliantly. Their clear, comprehensive, and readable textbook will guide astrophysicists and other interested scientists all the way to the frontiers of this exciting field.' Michael Fall, Space Telescope Science Institute, Baltimore

Daugiau informacijos

A comprehensive examination of nearly fourteen billion years of galaxy formation and evolution, from primordial gas to present-day galaxies.
Preface xi
1 Introduction
1(12)
1.1 Galaxies: a Very Brief History
1(2)
1.2 Galaxies as Astrophysical Laboratories
3(1)
1.3 Galaxies in the Cosmological Context
4(2)
1.4 Galaxies: from First Light to Present-Day Galaxies
6(3)
1.5 Galaxies: Near and Far, Now and Then
9(2)
1.6 Galaxies: the Emerging Picture and the Road Ahead
11(2)
2 The Cosmological Framework
13(15)
2.1 The Expanding Universe
13(5)
2.2 Dynamics of the Universe
18(2)
2.3 Standard Cosmological Model
20(4)
2.4 Cosmic Microwave Background, Recombination and Reionisation
24(2)
2.5 Big Bang Nucleosynthesis
26(1)
2.6 Thermal History of the Universe
27(1)
3 Present-Day Galaxies as a Benchmark for Evolutionary Studies
28(26)
3.1 Morphology
28(6)
3.2 Spectral Energy Distributions
34(2)
3.3 Integrated Radiation from Galaxies
36(1)
3.4 Galaxy Spectra
37(5)
3.5 Statistical Distributions of Galaxy Properties
42(6)
3.6 Active Galactic Nuclei
48(6)
4 Present-Day Star-Forming Galaxies
54(71)
4.1 Stars
54(11)
4.2 The Interstellar Medium of Star-Forming Galaxies
65(22)
4.3 Mass Distribution
87(12)
4.4 Scaling Relations
99(8)
4.5 Starburst Galaxies
107(1)
4.6 The Milky Way
108(17)
5 Present-Day Early-Type Galaxies
125(38)
5.1 Stars
126(15)
5.2 Diffuse Matter
141(4)
5.3 Mass Distribution
145(11)
5.4 Structural and Kinematic Scaling Relations
156(7)
6 The Environment of Present-Day Galaxies
163(32)
6.1 Interacting Galaxies
163(2)
6.2 Groups of Galaxies
165(2)
6.3 The Local Group
167(7)
6.4 Clusters of Galaxies
174(12)
6.5 The Influence of the Environment on Galaxy Properties
186(2)
6.6 Large-Scale Structure and Galaxy Clustering
188(3)
6.7 Baryon Budget
191(4)
7 Formation, Evolution and Properties of Dark Matter Halos
195(30)
7.1 Observational Evidence for Dark Matter Halos
195(1)
7.2 Dark Matter and Structure Formation
196(2)
7.3 Evolution of a Density Perturbation
198(7)
7.4 Statistical Properties of Cosmological Perturbations and Dark Matter Halos
205(8)
7.5 Structural and Kinematic Properties of Dark Matter Halos
213(12)
8 Main Ingredients of Galaxy Formation Theory
225(85)
8.1 Thermal Properties of Astrophysical Gases
225(9)
8.2 Gas Accretion and Cooling in Dark Matter Halos
234(7)
8.3 Star Formation
241(25)
8.4 Gas Consumption and Evolution of the Interstellar Medium
266(4)
8.5 Chemical Evolution
270(6)
8.6 Theoretical Spectra of Evolving Galaxies
276(8)
8.7 Feedback from Stars
284(8)
8.8 Feedback from Active Galactic Nuclei
292(7)
8.9 Merging of Galaxies
299(11)
9 From Recombination to Reionisation
310(40)
9.1 The Cosmological Recombination
310(5)
9.2 The Pregalactic Gas in the Dark Ages
315(1)
9.3 The Collapse of the Pregalactic Gas
316(1)
9.4 The Cooling of Primordial Gas
317(4)
9.5 Population III Stars
321(7)
9.6 From First Stars to First Galaxies
328(1)
9.7 The Formation of the First Massive Black Holes
329(2)
9.8 The Intergalactic Medium
331(7)
9.9 The Cosmological Reionisation
338(5)
9.10 Observing the Primeval Universe
343(7)
10 Theory of Galaxy Formation
350(72)
10.1 Formation of Galaxy Components: Discs
350(15)
10.2 Formation of Galaxy Components: Bars and Pseudobulges
365(4)
10.3 Formation of Galaxy Components: Spheroids
369(6)
10.4 Formation of Galaxy Components: Stellar Halos
375(1)
10.5 Characteristic Scales in Galaxy Formation
376(1)
10.6 Quenching of Star Formation
377(3)
10.7 Assembly History of Present-Day Star-Forming Galaxies
380(15)
10.8 Assembly History of Present-Day Early-Type Galaxies
395(6)
10.9 Formation of Dwarf Galaxies
401(2)
10.10 Origin of the Demographics of Present-Day Galaxies
403(12)
10.11 Numerical Models of Galaxy Formation
415(7)
11 Observing Galaxy Evolution
422(75)
11.1 The Main Observables of Galaxy Evolution
422(19)
11.2 The Difficult Observation of Distant Galaxies
441(29)
11.3 The Observation of Galaxy Evolution
470(24)
11.4 Summary
494(3)
Appendix A Acronyms 497(3)
Appendix B Constants and Units 500(2)
Appendix C Astronomical Compendium 502(18)
Appendix D Physics Compendium 520(13)
References 533(22)
Index 555
Andrea Cimatti is full Professor of Astrophysics at the Universitą di Bologna. He has worked in Germany, the USA, and Italy at the INAF Arcetri Astrophysical Observatory. His research uses the largest telescopes in space and on Earth to study galaxies and cosmology. He is one of the founders of ESA's Euclid space mission. He is a recipient of the Bessel Prize of the Alexander von Humboldt Foundation, among others. He teaches courses on fundamental astronomy and on galaxy formation and evolution. He has published key papers based on observational studies of distant galaxies. Filippo Fraternali is Associate Professor of Gas Dynamics and Evolution of Galaxies at the Kapteyn Astronomical Institute of the Rijksuniversiteit Groningen, The Netherlands. He obtained his Ph.D. from the Universitą di Bologna, where he was an assistant professor between 2006 and 2017. He did postdoctoral research in the Netherlands and was a Marie-Curie fellow at the University of Oxford. He has published extensively on various topics of galaxy formation and evolution. Carlo Nipoti is Associate Professor of Astrophysics at the Universitą di Bologna, where he received his Ph.D. in Astronomy, and he was a temporary lecturer of Theoretical Physics at the University of Oxford. He teaches courses on the physics of galaxies and on the dynamics of astrophysical systems at undergraduate and graduate levels. His research is in the field of theoretical astrophysics with special interest in the formation, evolution and dynamics of galaxies, on which he is author of valuable papers.