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| Àâòîðèçàöèÿ |
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| Ïîèñê ïî óêàçàòåëÿì |
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| Shore S.N. — The Tapestry of Modern Astrophysics |
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| Ïðåäìåòíûé óêàçàòåëü |
Entropy, Shannon form of 152
Epicyclic frequency 652—654 657
Equation of state, Bose — Einstein 34
Equation of state, cosmological 768—769 779—781
Equation of state, degenerate, nonrelativistic 28 31
Equation of state, degenerate, relativistic 29 31 33
Equation of state, Fermi — Dirac 32
Equation of state, ideal 18
Equation of state, partial ionization and 288—289
Equation of state, polytropic 285—289 324
Equation of state, radiation-dominated 286—288
Equation, Abel 731—732
Equation, agglomeration 68—69 519
Equation, Bernoulli 43
Equation, Boltzmann 54—55 66 67—68 210—211
Equation, Clausius — Mossotti 501
Equation, continuity 41 49 54 293
Equation, diffusion 438
Equation, Einstein field 89
Equation, Euler — Lagrange 76
Equation, Fokker — Planck 64—67 532 712
Equation, Friedmann — Robertson — Walker 766—767 774—775 777—781 819—821
Equation, hydrostatic 227
Equation, Killing 97—98
Equation, Kompaneets 209—214
Equation, Lane — Emden 38 294—299 646 724
Equation, linear adiabatic wave 326
Equation, linear pulsation 323—328
Equation, Malthus — Verhust 684
Equation, Mattig 785
Equation, Milne 183 269
Equation, Navier — Stokes 44
Equation, Oppenheimer — Volkoff 390
Equation, Poisson 4 5 37—38
Equation, radiative transfer see “Radiative transfer equation”
Equation, Saha 36 773
Equation, Tolman — Oppenheimer — Volkoff 390
Equation, Vlasov 40—43 642—644
Equations of motion, conservative form 42
Equations of motion, Euler — Lagrange 76
Equations of motion, fluid 41—42 49 555
Equations of motion, Hamiltonian 20
Equations of motion, stellar hydrodynamics 643—644
Equivalence principle 86
Equivalent width 202 480
Escape probability 256—259
Euler — Lagrange equation 76
Exponential integrals 183
Extinction 180 498—500
Extinction and column densities 500
Extinction and polarization 514
Extrasolar planetary systems, eclipsing 415
Faber — Jackson relation 748—749
Fanaroff — Riley classification for radio galaxies 713—714
Faraday depth 539
Faraday rotation 515 536—540
Fermi Golden Rule 262
Fermi momentum 28
Fermi process 528—529
Fermi — Dirac distribution see “Distribution function Fermi
Fermi — Dirac integral, defined 32
fermions see “Distribution function Fermi
Fick’s law see “Diffusion Fick’s
Finesse 138
Fluorescence 205—207 463
Flux see “Radiative flux”
Fokker — Planck equation 64—67 532 712
Forbidden line transitions 462—466 472 747
Fossil Stroemgren sphere 571
Fourier transform 155 162—163 439 “Power
Free energy see “Thermodynamics free “Partition
Free-free opacity see “Opacity thermal
Friedmann — Robertson — Walker (FRW) metric see “Metric Friedmann
Friedmann — Robertson — Walker equations 766—767 774—775 777—781
Friedmann — Robertson — Walker equations, perturbed form 819—821
Fringe visibility see “Interferometers visibility”
Fugacity 30
Fullerenes 553
Fundamental plane see “Elliptical galaxies fundamental
Galaxies, active galactic nuclei (AGN) 700—703
Galaxies, bars 666—668 691—692
Galaxies, chemical evolution of see “Chemical evolution of galaxies”
Galaxies, Elliptical 692—695 720
Galaxies, escape velocity from 698—699
Galaxies, galactic winds 686—687
Galaxies, Hubble classification 690—697
Galaxies, infall of gas 686—688
Galaxies, irregular 695—697 804—805
Galaxies, polar ring 716—717
Galaxies, ring 716—718
Galaxies, rotation curves 655—660 697—700 733 747—748
Galaxies, Spiral 690—692
Galaxies, spiral structure 661—668
Galaxies, tidal interactions 685
Galaxy clusters see “Clusters of galaxies”
Galaxy, galactic center 640 704—705
Galaxy, galactic coordinates 640 655—658
Galaxy, rotation law 655—660
Galaxy, solar galactocentric distance 650—651
Galaxy, spiral structure 660—661 (see also “Density waves”)
Galaxy, surface mass density 645
Galaxy, vertical structure of disk 644—647 653 657—658
Galilean transformation 556
Galileo and astronomical measurements 104—105
Gamma ray bursts 842—844
Gamow factor 332
Gaunt factor 194
Gaussian process see “Random processes Gaussian”
Gauss’ Theorem 4
General relativity 81—102
General relativity, principle of covariance 79 83
Geodesic 85
Giant branch 372—374 (see also “Hayashi track”)
Gibbs free energy see “Thermodynamics Gibbs
Glitch 399—400
Globular clusters 635—637
Gould belt 651—652 654 672 685
Gravitational contraction as energy source 329—330
Gravitational deflection of light see “Gravitational lens”
Gravitational lens 95 98—99
Gravitational lens and clusters of galaxies 730—731
Gravitational lens and galactic halo objects (MACHOs) 647—648
Gravitational lens, image formed by extended mass distribution 836—841
Gravitational lens, magnification 839
Gravitational potential 4—5 57 70—75
Gravitational potential, classical spheroids 70—75
Gravitational potential, Maclaurin spheroid 74—75 455 693—694
Gravitational waves 99—101 428—430 834—836
Gravitational waves, detection of 101
Gravitational waves, emission by close binary system 428—430
Gravitothermal catastrophe 62 289—290
Gravity darkening 238—239 308 420
Green function 5
Gunn — Peterson test 796 824
Gyrosynchrotron process 535—536
H II regions see “Champagne flow” “Stroemgren
H II regions as shocks 565—567 572—573
H II regions, compact 571
H II regions, fossil 571
H II regions, static 567—568
H theorem 67—68 (see also “Boltzmann equation”)
Halley — Olbers dark sky paradox 806—807
Hamiltonian equations of motion 20
Hanle effect 216
Harmonic Law see “Kepler’s Law”
Harrison — Peebles — Zel’dovich spectrum 829
Harvard spectral classification 225
Hauser — Feshbach method 337
Hayashi track 368—369 372—373
Helioseismology 320—323
| Helium flash 372—373 (see also “Thermonuclear reactions” “Thermonuclear
Helmholtz free energy see “Thermodynamics Helmholtz
Henry Draper Catalog (HD) see “Harvard spectral classification”
Hertzsprung — Russell diagram (HR diagram) 359 631—633
Hickson compact groups see “Clusters of galaxies”
Hipparchos satellite 107 and passim
Historical notes, Astrophysical Journal 166
Historical notes, binary and multiple stars 412—413
Historical notes, convection 302
Historical notes, cosmological constant 775
Historical notes, cosmology 734—740
Historical notes, dust in the interstellar medium 495—498
Historical notes, expanding H II regions 571—572
Historical notes, galaxies 689—690
Historical notes, Galaxy 629—630
Historical notes, Hertzsprung — Russell diagram and stellar evolution 357—359
Historical notes, interstellar medium 459—461
Historical notes, pulsars 394
Historical notes, spectral classification 225—226 272—274
Historical notes, stellar structure and evolution 281—282 294
Historical notes, stellar thermonuclear energy 337
Historical notes, synchrotron emission 533
Historical notes, thermonuclear instabilities 374
Historical notes, URCA process 357
Homology relations 309—310
Hopf function 183 271—272
Horizon distance 786—790
Horizons and black holes 93—97
Horizons and cosmology 783—790
Hubble classification of galaxies 690—697
Hubble constant 752 764
Hubble flow 576
Hubble parameter (H) 754
Hydrogen burning 337—341 348 375
Hydrogen,  549—550
Hydrogen, 21 cm line of H I 482—485 500 658—659 673
Hydrogen, hydrogen line profiles and pressure broadening 220—222
Hydrogen, Lyman lines 476—477 482 500 797—798
Hydrogen, molecular formation 544—546
Hydrogen, molecular hydrogen lines 490—491 500
Hydrostatic equation as function of optical depth 227
Hydrostatic equilibrium 227 293 724
Hydrostatic equilibrium for accretion disk 436
Hyperfine structure 214—215
Ideal gas law 18
Image reconstruction methods 146—156
Impact approximation see “Stark effect quantum
Impact parameter 39
Inertial subrange 604—605
Inflation 781—783 789—795
Initial mass function (IMF) 404—405 672—673
Instabilities, Alfven waves 50—51
Instabilities, convection 302—306
Instabilities, gravitoacoustic 582—586 663—665 818—822 826—830
Instabilities, Jeans see “Instabilities gravitoacoustic”
Instabilities, Kelvin — Helmholtz 582
Instabilities, magnetorotational (MRI) 442—445
Instabilities, Parker 600—602 618—620
Instabilities, pulsational 311—328
Instabilities, Rayleigh — Taylor 582 600
Instabilities, Richtmyer — Meshkov 582
Instabilities, sound (acoustic) 44—46 835
Instabilities, thermal 590—597 724—728
Instantaneous recycling approximation 677—680
Intensity, integrated (J) 176—177
Intensity, specific 167
Interferometers, Fabry — Perot 138—139
Interferometers, image formation 134 140—142
Interferometers, intensity 139
Interferometers, Michelson 137—138
Interferometers, speckle 145
Interferometers, visibility 137
Intermittency 612—613
Invariant imbedding 265—268
Ionization equilibrium, Saha equation 35—36
Ionization parameter 570
Ionization, collisional 172 547
Ionization, effect of partial ionization on equation of state 288—289
Ionization, energies for atomic species 195
Ionization, photoionization see “Photoionization”
Irregular galaxies see “Galaxies irregular”
Isochrones 401—404 631—637 673—674
Isothermal disk 645—647 698
Isothermal sphere see “Lane — Emden equation isothermal” “King
Isotopes, isotopic fractionation 550—552 (see also “Radionuclides”)
J shocks see “Magnetic fields and shocks”
Jansky, defined 129
Jeans escape see “Outflows thermal
Jeans instability see “Instabilities gravitoacoustic”
Jeans length and mass 585
K correction 756
Kelvin — Helmholtz contraction 329—330 365—366
Kelvin — Helmholtz contraction, timescale 61 284
Kepler’s law 3
Killing equation 97—98
King model 698 724
Kirchhoff — Bunsen laws 173
Klein — Nishima formula 209
Kolmogorov length 604
Kolmogorov spectrum see “Turbulence Kolmogorov
Kompaneets equation 209—214 (see also “Scattering Compton”)
Lagrange multipliers 24 152 159—160
Lagrangian frame 263
Lagrangian points 12—13 418—420 666—668
Lambda iteration 232
Lane — Emden equation 294—299
Lane — Emden equation, isothermal 38 298 646 724
Langevin rate 546
Large velocity gradient method see “Sobolev approximation”
Larmor formula 615
Larmor frequency 47
Larson — Penston law for isothermal sphere 598
Least action principle 76
Lenticular galaxies see “Galaxies spiral”
Light echo 520—521
Light element synthesis 680—682 801—805
Likelihood 151 160
Limb darkening 184—186
Limb darkening and eclipsing binary light curves 120 414
Limb darkening and rotational broadening of line profiles 222—223
Limb darkening, coefficient 185
Lindblad resonances 662—665
Line profile, broadening 214—224
Line profile, damped 203 478—481
Line profile, damping factor 198—199 217
Line profile, function 169
Line profile, Gaussian 199 478
Line profile, Holtzmark 217—218
Line profile, Lorentzian 198 476—482
Line profile, P Cygni 253—255
Line profile, pressure gradients from line wings 220—222
Line profile, redistribution in 205
Line profile, rotational 222—223
Line profile, saturated 202 480—481
Line profile, Voigt 200—201 478—482
Linear adiabatic wave equation 326
LINER (low ionization emission line galaxies) see “Galaxies active
Local Group see “Clusters of galaxies Local
Local standard of rest (LSR) 640—641 644
Local thermodynamic equilibrium (LTE), defined 36—37 (see also “Non-LTE conditions
Lomb — Scargle method for time series 148—149
Lookback time 785
Lorentz factor ( ) 78 91
Lorentz force 47 80
Lorentz invariance 78—79
Lorentz transformations 78—79
Lutz — Keller bias 108—109
Lyman alpha forest 415 417 476—482 797—798
Lyman limit 194
Mach number 557
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