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Extragalactic Astronomy and Cosmology: An Introduction

Extragalactic Astronomy and Cosmology: An Introduction

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Subject Index<br />

454<br />

321–324<br />

– Abell catalog 228–230<br />

– Abell radius 229<br />

– baryon content 323<br />

– beta-model 261<br />

– catalogs 228–230, 255–256, 322<br />

– classification 231<br />

– color–magnitude diagram 271<br />

– Coma cluster 12, 228, 242<br />

– cooling flows 248–252, 263, 401<br />

– core radius 232, 233<br />

– dark matter 223, 234, 248, 323<br />

– distance class 230<br />

– evolution effects 270–273<br />

– galaxy distribution 231–233<br />

– galaxy luminosity function 230<br />

– galaxy population 393<br />

– HIFLUGCS catalog 255, 256<br />

– hydrogen clouds 237<br />

– intergalactic stars 236–237<br />

– intracluster medium 223, 236,<br />

242–256<br />

– luminosity function 256, 270<br />

– mass determination 13, 233–234,<br />

246, 248, 257, 262, 266, 322<br />

– mass–luminosity relation 258<br />

– mass–temperature relation 256<br />

– mass-to-light ratio 234, 266<br />

– mass–velocity dispersion relation<br />

257<br />

– morphology 231<br />

– near-infrared luminosity 259<br />

– normalization of the power spectrum<br />

291, 322, 324<br />

– number density 322, 330<br />

– projection effects 229, 255<br />

– richness class 230<br />

– scaling relations 256–260, 322<br />

– Virgo Cluster 12, 228<br />

– X-ray radiation 13<br />

– Zwicky catalog 229<br />

COBE 22, 168, 336, 341, 346<br />

cold dark matter (CDM) 286<br />

– substructure 396<br />

collisionless gas 94<br />

color excess 41<br />

color filter 420–422<br />

color index 41, 420<br />

color temperature 425<br />

color–magnitude diagram 39, 373,<br />

425<br />

Coma cluster of galaxies 12, 117, 228<br />

comoving coordinates 146, 280<br />

comoving observers 146, 155<br />

Compton Gamma Ray Observatory<br />

(CGRO) 32, 402<br />

Compton scattering 193<br />

– inverse 168, 193, 214, 252, 381<br />

concentration index of the NFW profile<br />

299<br />

convection 427<br />

convergence point 38<br />

cooling fronts 251<br />

cooling of gas 384, 391, 396<br />

– <strong>and</strong> star formation 384, 396<br />

– the role of molecular hydrogen 384<br />

Copernicus satellite 30<br />

correlation function 283–284, 288,<br />

316, 338, 360, 398<br />

– related to biasing 358<br />

correlation length 283<br />

cosmic microwave background 3, 16,<br />

142, 252, 253, 336, 379<br />

– dipole 114, 316, 320<br />

– discovery 168, 336<br />

– fluctuations 277, 278, 309,<br />

336–349<br />

– foreground emission 342<br />

– measuring the anisotropy 341–349<br />

– origin 168<br />

– polarization 307, 348<br />

– primary anisotropies 336–337<br />

– redshift evolution 156<br />

– secondary anisotropies 336–338,<br />

341<br />

– spectrum 156, 381, 383<br />

– temperature 156<br />

cosmic rays 51–54, 180<br />

– acceleration 53<br />

– energy density 54<br />

cosmic shear see gravitational lenses<br />

cosmic variance 346–347<br />

cosmological constant 4, 15, 148,<br />

149, 327, 344, 349<br />

cosmological parameters,<br />

determination 291, 309–355<br />

cosmological principle 145<br />

cosmology 14, 17, 141–174, 309,<br />

277–354<br />

– components of the Universe<br />

149–151<br />

– curvature scalar 151<br />

– density fluctuations 145, 277–335<br />

– expansion equation 147, 149–155<br />

– expansion rate 146, 155<br />

– homogeneous world models<br />

141–174<br />

– Newtonian cosmology 146–148<br />

– structure formation 16, 17, 279,<br />

391<br />

COSMOS survey 367<br />

D<br />

D n –σ relation 108<br />

dark energy 4, 149, 327, 328, 353,<br />

412<br />

dark matter 3, 63, 64, 102, 165–166,<br />

353, 411–412<br />

– cold <strong>and</strong> hot dark matter 286–287,<br />

351, 391<br />

– in clusters of galaxies 13, 223, 248<br />

– in galaxies 8, 100, 101<br />

– in the Universe 17, 165, 281, 336<br />

dark matter halos 101, 290–293, 391<br />

– number density 291–293, 322, 383<br />

– substructure 302–306<br />

– universal mass profile 298–302<br />

de Vaucouleurs law 55, 90, 98<br />

deceleration parameter 153, 154<br />

declination 35<br />

deflection of light see gravitational<br />

lenses<br />

density contrast 278, 289<br />

density fluctuations in the Universe<br />

277<br />

– origin 307<br />

density parameter 148, 151, 154, 171,<br />

322, 330, 336, 344, 349, 351, 353<br />

deuterium 163<br />

– in QSO absorption lines 165<br />

– primordial 165<br />

diskiness in elliptical galaxies 96<br />

distance determination 114, 253<br />

– of extragalactic objects 104,<br />

114–117<br />

– within the Milky Way 36–44<br />

distance ladder 114<br />

distance modulus 40, 422<br />

distances in cosmology 155,<br />

157–159, 216<br />

Doppler broadening 196

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