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Peter Schneider Extragalactic Astronomy <strong>and</strong> <strong>Cosmology</strong> An Introduction With 446 figures, including 266 color figures 123
Page 2: Peter Schneider Extragalactic Astro
Page 10: Preface V This book began as a seri
Page 14: List of Contents VII 1. Introductio
Page 18: List of Contents IX 3.8 Galaxies as
Page 22: List of Contents XI 6.2.4 Spatial D
Page 26: List of Contents XIII 9.2 New Types
Page 30: 1. Introduction and Overview 1 1.1
Page 34: 1.1 Introduction a crucial role in
Page 38: 1.2 Overview 5 250 Rotation Velocit
Page 42: 1.2 Overview parameters of the Milk
Page 46: 1.2 Overview Fig. 1.9. The spectra
Page 50: 1.2 Overview random velocities of t
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1.2 Overview Fig. 1.14. The Coma cl
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1.2 Overview • the current mean m
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1.2 Overview 17 The CMB photons we
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1.3 The Tools of Extragalactic Astr
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2. The Milky Way as a Galaxy 36 Fig
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2. The Milky Way as a Galaxy 38 ric
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2. The Milky Way as a Galaxy 40 tri
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2. The Milky Way as a Galaxy 44 gra
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2. The Milky Way as a Galaxy 46 A s
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2. The Milky Way as a Galaxy 48 a l
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2. The Milky Way as a Galaxy 50 iro
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2. The Milky Way as a Galaxy 52 is
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2. The Milky Way as a Galaxy 54 is
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2. The Milky Way as a Galaxy 56 The
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2. The Milky Way as a Galaxy 58 whe
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2. The Milky Way as a Galaxy 60 If
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2. The Milky Way as a Galaxy 62 Con
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2. The Milky Way as a Galaxy 66 The
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2. The Milky Way as a Galaxy 68 fac
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2. The Milky Way as a Galaxy 70 the
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2. The Milky Way as a Galaxy 72 nif
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2. The Milky Way as a Galaxy 74 pro
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2. The Milky Way as a Galaxy 78 bee
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2. The Milky Way as a Galaxy 84 any
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3. The World of Galaxies 87 The ins
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3.1 Classification these names are
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3.2 Elliptical Galaxies 91 Fig. 3.5
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3.2 Elliptical Galaxies 93 Fig. 3.7
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3.2 Elliptical Galaxies anisotropic
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3.2 Elliptical Galaxies Fig. 3.12.
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3.3 Spiral Galaxies 99 Fig. 3.14. T
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3.3 Spiral Galaxies 101 Fig. 3.15.
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3.3 Spiral Galaxies luminous galaxi
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3.4 Scaling Relations 105 Fig. 3.20
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3.4 Scaling Relations gas, which ca
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3.5 Black Holes in the Centers of G
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3.5 Black Holes in the Centers of G
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3.6 Extragalactic Distance Determin
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3.6 Extragalactic Distance Determin
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3.7 Luminosity Function of Galaxies
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3.7 Luminosity Function of Galaxies
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3.8 Galaxies as Gravitational Lense
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3.9 Population Synthesis 131 Fig. 3
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3.9 Population Synthesis The integr
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3.9 Population Synthesis photometri
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3.9 Population Synthesis 137 Fig. 3
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3.10 Chemical Evolution of Galaxies
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4. Cosmology I: Homogeneous Isotrop
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4.1 Introduction and Fundamental Ob
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4.2 An Expanding Universe the Hubbl
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4.2 An Expanding Universe in which
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4.2 An Expanding Universe physical
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4.2 An Expanding Universe time. Hen
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4.3 Consequences of the Friedmann E
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4.4 Thermal History of the Universe
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4.5 Achievements and Problems of th
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5. Active Galactic Nuclei 175 The l
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5.1 Introduction 5.1 Introduction 5
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5.1 Introduction 179 Fig. 5.5. Radi
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5.1 Introduction The synchrotron sp
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5.2 AGN Zoology have in common stro
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5.3 The Central Engine: A Black Hol
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5.4 Components of an AGN 5.4 Compon
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5.4 Components of an AGN transition
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5.4 Components of an AGN Fig. 5.22.
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5.4 Components of an AGN by magneti
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5.4 Components of an AGN sible to o
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5.4 Components of an AGN ity of an
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5. Active Galactic Nuclei 208 radia
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5. Active Galactic Nuclei 210 Fig.
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5. Active Galactic Nuclei 212 5.5.4
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5. Active Galactic Nuclei 214 elect
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5. Active Galactic Nuclei 216 QSOs
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5. Active Galactic Nuclei 218 tion.
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5.6 AGNs and Cosmology 221 ize hydr
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6. Clusters and Groups of Galaxies
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6.1 The Local Group 225 Table 6.1.
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7. Cosmology II: Inhomogeneities in
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7.2 Gravitational Instability gravi
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7.2 Gravitational Instability i.e.,
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7.3 Description of Density Fluctuat
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7.4 Evolution of Density Fluctuatio
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7.4 Evolution of Density Fluctuatio
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7.5 Non-Linear Structure Evolution
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7.7 Origin of the Density Fluctuati
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8. Cosmology III: The Cosmological
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352 8. Cosmology III: The Cosmologi
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9. The Universe at High Redshift 35
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10. Outlook 407 In the final chapte
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10. Outlook telescope will start a
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10. Outlook New windows to the Univ
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10. Outlook understand why the dens
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Appendix
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A. The Electromagnetic Radiation Fi
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B. Properties of Stars 425 In this
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B.3 Structure and Evolution of Star
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B.3 Structure and Evolution of Star
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D. Recommended Literature 433 In th
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D.3 Review Articles, Current Litera
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E. Acronyms Used 438 GRB Gamma-Ray
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F. Figure Credits 441 Chapter 1 1.1
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F. Figure Credits 1.25 Source: R. W
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F. Figure Credits Nik Szymanek. bot
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F. Figure Credits 5.5 Credit: Laing
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F. Figure Credits 6.26 Source: http
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F. Figure Credits 8.24 Credit: Hu &
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Subject Index 453 A AB magnitudes 4
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Subject Index 455 Doppler effect 38
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Subject Index 457 -dampedLyα syste
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Subject Index 459 virial theorem 13
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