and Cosmology
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