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E. Acronyms Used 437 In this appendix, we compile some of the acronyms that are used, and references to the sections in which these acronyms have been introduces or explained. 2dF(GRS) Two-Degree Field Galaxy Redshift Survey (Sect. 8.1.2) ACBAR Arcminute Cosmology Bolometer Array Receiver (Sect. 8.6.5) ACO Abell, Corwin & Olowin (catalog of clusters of galaxies, Sect. 6.2.1) ACS Advanced Camera for Surveys (HST instrument) AGB Asymptotic Giant Branch (Sect. 3.9.2) AGN Active Galactic Nucleus (Chap. 5) ALMA Atacama Large Millimeter Array (Chap. 10) APEX Atacama Pathfinder Experiment (Chap. 10) AU Astronomical Unit BAL Broad Absorption Line (-Quasar, Sect. 5.6.3) BATSE Burst And Transient Source Experiment (CGRO instrument, Sect. 9.7) BBB Big Blue Bump (Sect. 5.4.1) BBN Big Bang Nucleosynthesis (Sect. 4.4.4) BCD Blue Compact Dwarf (Sect. 3.2.1) BH Black Hole (Sect. 5.3.5) BLR Broad-Line Region (Sect. 5.4.2) BLRG Broad-Line Radio Galaxy (Sect. 5.2.3) BOOMERANG Balloon Observations Of Millimetric Extragalactic Radiation and Geophysics (Sect. 8.6.4) CBI Cosmic Background Imager (Sect. 8.6.5) CCD Charge Coupled Device CDM Cold Dark Matter (Sect. 7.4.1) CERN Conseil European pour la Recherché Nucleaire CfA Harvard–Smithsonian Center for Astrophysics CFHT Canada–France–Hawaii Telescope (Sect. 1.3.3) CFRS Canada–France Redshift Survey (Sect. 8.1.2) CGRO Compton Gamma Ray Observatory (Sect. 1.3.5) CHVC Compact High-Velocity Cloud (Sect. 6.1.3) CIB Cosmic Infrared Background (Sect. 9.3.1) CLASS Cosmic Lens All-Sky Survey (Sect. 3.8.3) CMB Cosmic Microwave Background (Sect. 8.6) CMD Color–Magnitude Diagram (Appendix B) COBE Cosmic Background Explorer (Sect. 8.6.4) CTIO Cerro Tololo Inter-American Observatory DASI Degree Angular Scale Interferometer (Sect. 8.6.4) EdS Einstein–de Sitter (Sect. 4.3.4) EMSS Extended Medium Sensitivity Survey (Sect. 6.3.5) EPIC European Photon Imaging Camera EROS (XMM-Newton instrument) Expérience pour la Recherche d’Objets Sombres (microlenses collaboration, Sect. 2.5) ESA European Space Agency ESO European Southern Observatory (Sect. 1.3.3) FFT Fast Fourier Transform (Sect. 7.5.3) FIR Far Infrared FJ Faber–Jackson (Sect. 3.4.2) FOC Faint Object Camera (HST instrument) FORS Focal Reducer / Low Dispersion Spectrograph (VLT instrument) FOS Faint Object Spectrograph (HST instrument) FP Fundamental Plane (Sect. 3.4.3) FR(I/II) Faranoff–Riley Type (Sect. 5.1.2) FWHM Full Width Half Maximum GC Galactic Center (Sect. 2.3, 2.6) Peter Schneider, Acronyms Used. In: Peter Schneider, Extragalactic Astronomy and Cosmology. pp. 437–439 (2006) DOI: 10.1007/11614371_E © Springer-Verlag Berlin Heidelberg 2006
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Peter Schneider Extragalactic Astro
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Prof. Dr. Peter Schneider Argelande
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Preface VI ter aspects are discusse
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List of Contents VIII 2.5.1 The Gra
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List of Contents X 5. Active Galact
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List of Contents XII 8. Cosmology I
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List of Contents XIV D. Recommended
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1. Introduction and Overview 2 Fig.
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1. Introduction and Overview 4 othe
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1. Introduction and Overview 6 obje
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1. Introduction and Overview 8 Fig.
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1. Introduction and Overview 10 Fig
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1. Introduction and Overview 16 of
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1. Introduction and Overview 18 app
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1. Introduction and Overview 26 spe
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2. The Milky Way as a Galaxy 35 The
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2.2 Determination of Distances With
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2.3 The Structure of the Galaxy Fig
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2.3 The Structure of the Galaxy a c
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2.3 The Structure of the Galaxy Fig
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2.3 The Structure of the Galaxy B-s
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2.3 The Structure of the Galaxy Fro
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2.3 The Structure of the Galaxy tha
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2.4 Kinematics of the Galaxy 57 2.4
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2.4 Kinematics of the Galaxy which
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2.4 Kinematics of the Galaxy where
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2.4 Kinematics of the Galaxy center
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2.5 The Galactic Microlensing Effec
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2.6 The Galactic Center have been e
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2.6 The Galactic Center 79 Fig. 2.3
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2.6 The Galactic Center Fig. 2.36.
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2.6 The Galactic Center 83 Fig. 2.3
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2.6 The Galactic Center hence, this
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3. The World of Galaxies 88 million
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3. The World of Galaxies 90 100M
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3. The World of Galaxies 92 Table 3
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3. The World of Galaxies 94 arrives
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96 3. The World of Galaxies This in
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3. The World of Galaxies 98 Boxines
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3. The World of Galaxies 100 Wherea
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3. The World of Galaxies 102 the po
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3. The World of Galaxies 104 The ki
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3. The World of Galaxies 106 Fig. 3
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3. The World of Galaxies 108 where
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3. The World of Galaxies 110 angula
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3. The World of Galaxies 116 LMC sh
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3. The World of Galaxies 118 should
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3. The World of Galaxies 124 The de
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3. The World of Galaxies 130 An eve
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3. The World of Galaxies 132 3.9 Po
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3. The World of Galaxies 136 3.9.4
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3. The World of Galaxies 140 by no
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4. Cosmology I: Homogeneous Isotrop
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5. Active Galactic Nuclei 176 Fig.
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5. Active Galactic Nuclei 178 the r
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5. Active Galactic Nuclei 180 of re
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5. Active Galactic Nuclei 182 emiss
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5. Active Galactic Nuclei 184 surve
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5. Active Galactic Nuclei 186 chang
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188 5. Active Galactic Nuclei diffe
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5. Active Galactic Nuclei 194 For a
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5. Active Galactic Nuclei 196 5.4.2
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5. Active Galactic Nuclei 198 wheth
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5. Active Galactic Nuclei 202 There
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5. Active Galactic Nuclei 204 Binar
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5.5 Family Relations of AGNs ing t
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5.5 Family Relations of AGNs 209 Fi
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5.5 Family Relations of AGNs relati
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5.5 Family Relations of AGNs 213 Fi
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5.6 AGNs and Cosmology a given freq
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5.6 AGNs and Cosmology Φ(L, z) dL
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5.6 AGNs and Cosmology at very high
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5. Active Galactic Nuclei 222 QSO w
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6. Clusters and Groups of Galaxies
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6. Clusters and Groups of Galaxies
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6.2 Galaxies in Clusters and Groups
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6.3 X-Ray Radiation from Clusters o
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6.4 Scaling Relations for Clusters
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6.4 Scaling Relations for Clusters
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6.5 Clusters of Galaxies as Gravita
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6.6 Evolutionary Effects M/L ≈ 80
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6.6 Evolutionary Effects 271 Fig. 6
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6.6 Evolutionary Effects Fig. 6.45.
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6.6 Evolutionary Effects satellites
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7. Cosmology II: Inhomogeneities in
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280 7. Cosmology II: Inhomogeneitie
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8. Cosmology III: The Cosmological
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8.1 Redshift Surveys of Galaxies a
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8.1 Redshift Surveys of Galaxies SD
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8.1 Redshift Surveys of Galaxies 31
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Physical space Linear regime Redshi
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8.1 Redshift Surveys of Galaxies ie
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8.2 Cosmological Parameters from Cl
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8.2 Cosmological Parameters from Cl
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8.3 High-Redshift Supernovae and th
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8.3 High-Redshift Supernovae and th
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8.4 Cosmic Shear ity one can separa
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8.5 Origin of the Lyman-α Forest F
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8.5 Origin of the Lyman-α Forest p
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8.5 Origin of the Lyman-α Forest 3
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8.6 Angular Fluctuations of the Cos
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8.7 Cosmological Parameters smaller
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8.7 Cosmological Parameters Fig. 8.
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8.7 Cosmological Parameters measure
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9. The Universe at High Redshift 35
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9.1 Galaxies at High Redshift one e
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9.1 Galaxies at High Redshift Fig.
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9.1 Galaxies at High Redshift neutr
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9.1 Galaxies at High Redshift break
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9.1 Galaxies at High Redshift to sc
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9.1 Galaxies at High Redshift the H
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9.2 New Types of Galaxies 369 Fig.
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9.2 New Types of Galaxies dust. A m
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9.2 New Types of Galaxies 373 Fig.
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9.2 New Types of Galaxies Fig. 9.21
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9.2 New Types of Galaxies tons whic
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9.3 Background Radiation at Smaller
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9.3 Background Radiation at Smaller
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9.4 Reionization of the Universe Th
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9.4 Reionization of the Universe 9.
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9.5 The Cosmic Star-Formation Histo
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9.5 The Cosmic Star-Formation Histo
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9.6 Galaxy Formation and Evolution
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9.7 Gamma-Ray Bursts 403 Fig. 9.41.
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9.7 Gamma-Ray Bursts Hypernovae. At
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10. Outlook 408 Fig. 10.2. The coll
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Page 904: E. Acronyms Used 438 GRB Gamma-Ray
Page 910: F. Figure Credits 441 Chapter 1 1.1
Page 914: F. Figure Credits 1.25 Source: R. W
Page 918: F. Figure Credits Nik Szymanek. bot
Page 922: F. Figure Credits 5.5 Credit: Laing
Page 926: F. Figure Credits 6.26 Source: http
Page 930: F. Figure Credits 8.24 Credit: Hu &
Page 934: Subject Index 453 A AB magnitudes 4
Page 938: Subject Index 455 Doppler effect 38
Page 942: Subject Index 457 -dampedLyα syste
Page 946: Subject Index 459 virial theorem 13
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