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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 |
Maclaurin spheroid see “Gravitational potential Maclaurin
Magellanic Stream 716
Magnetic fields and alignment of interstellar dust grains 514—518
Magnetic fields and coupling in accretion disks 442—445
Magnetic fields and shocks 558—565
Magnetic fields in active galactic nuclei 708—715
Magnetic fields in interstellar clouds 542—543 (see also “Ambipolar diffusion”)
Magnetic fields, ambipolar diffusion see “Ambipolar diffusion”
Magnetic fields, equipartition and minimum energy 708—711
Magnetic fields, frozen-in approximation 51 407
Magnetic fields, generation by dynamos 405—410
Magnetic fields, Hanlc effect 216
Magnetic fields, magnetospheres of accreting stars 450—452
Magnetic fields, maximum mass of magnetic clouds 588—589
Magnetic fields, measurements with Faraday rotation 537—540
Magnetic fields, molecular clouds see “Ambipolar diffusion”
Magnetic fields, pulsars see “Pulsars”
Magnetic fields, turbulent 606—607 609
Magnetic fields, Zeeman effect 215—216
magnetic susceptibility 517—518
Magneto hydrodynamics (MHD) 49—51
Magnetosonic waves 50—51
Magnetospheres 396—399 450—452
Magnitudes 109—112
Magnitudes, AB system, defined 114
Magnitudes, absolute 111
Magnitudes, astronomical, defined 109
Magnitudes, calibration zero point 109—110
Magnitudes, color index 118
Magnitudes, distance modulus 111
Magnitudes, Pogson’s ratio 109
Magnitudes, standard multicolor filter systems 112—117
Main sequence, chemical abundance anomalies in 248—249 276
Main sequence, lower mass cutoff 369
Main sequence, mass-luminosity relation 361—362
Main sequence, thermonuclear reactions during 337—341
Main sequence, turn-off 370 403
Main sequence, zero age (ZAMS) 367—368
Malmquist bias 807—808
Malthus — Verhust equation 684
MAMA see “Detectors multianode
Masers 175—176 491—492 705—706 749
Mass function see “Binary stars mass
Mass-luminosity relations 361—362
Mass-radius relations 367 380—382
Mathis — Rumpl — Nordsieck dust distribution 499—500 518—519
Matter-dominated cosmology 779—780
Mattig equation 785
Maximum entropy method (MEM) 151—154 159—160
Maxwellian distribution see “Distribution function Maxwellian”
Mean free path 38 52
mergers see “Tidal interactions galaxies”
Meridional circulation 308—309 341
Meteorites see “Radionuclides”
Meteorites, abundances 506 349—351 669—672
Metric 81—86
Metric and gravitational waves 100
Metric, Friedmann — Robertson — Walker 758—762
Metric, Minkowski 79 82
Metric, Schwarzschild 93 390
Metric, signature 82
Metric, symmetries 97—98 759—760
Michelson interferometer see “Interferometers Michelson”
Microturbulence 200 480—481
Mie scattering 501—503 521
Milky Way see “Galaxies” “Galaxy”
Milne equation (also called Schwarzschild — Milne equation) 183 269
Minkowski metric 79 82
Mixing in stellar interiors 375—377 (see also “Convection” “Meridional
Mixing length theory for convection 234—237 305—306
Molecular clouds, classification of 522—523
Molecular clouds, linewidth-velocity relation 524—525
Molecular clouds, turbulence in 608—612
Molecular lines, CO 523—524 548—549
Moments, velocity distribution 40—43 58—59
Monte-Carlo methods 190—192 257
Morgan — Keenan spectral classification 225
Multiphase interstellar medium 595—597
Multiplets 174
n-body problem 15
Navier — Stokes equation 44
Nebular diagnostics 462—472
Nebulium ([O III] lines) 462—463
Neutral buoyancy 236
Neutrinos 33—34
Neutrinos and stellar nucleosynthesis 351—352
Neutrinos, plasmon 351—352
Neutrinos, solar neutrinos 337—341 352—356
Neutrinos, URCA process 356—357 385 393—394
Neutron reactions 344—348 375—376
Neutron reactions, cosmological 799—802
Neutron reactions, r-process 346
Neutron reactions, s-process 345—346
Neutron stars 389—394
Neutron stars, cooling 393—394
Neutrons, lifetime, and cosmological nucleosynthesis 799
Neutrons, sources in stellar interiors 347—348 375—376
NLTE see “Non-LTE”
Noise-equivalent power (NEP) 130
Non-LTE (NLTE) see “Statistical equilibrium”
Non-LTE (NLTE), conditions for 237—238
Non-LTE (NLTE), masers 169—170 175—176
Non-LTE (NLTE), scattering 186—189
Non-LTE (NLTE), source function 179—180 187—188
Novae and cosmological distance scale 744—746
Novae as accreting binaries 448—450
Novae, common envelope stage 425
Novae, line formation in 259—260
Novae, thermonuclear runaway 448—450
Nuclear binding energy 330—331
Nuclear reactions, barrier penetration probability 332 334
Nuclear reactions, Breit — Wigner resonance 335
Nuclear reactions, compound nucleus 336 366—370
Nuclear reactions, Coulomb barrier 331
Nuclear reactions, Gamow factor 332
Nuclear reactions, nonresonant 336
Nuclear reactions, nuclear radius, scaling relation for 331
Nuclear reactions, S factor 332
Nuclear reactions, specific see “Thermonuclear reactions”
Nuclear reactions, two-body reaction rate, scaling law for 334
Nucleocosmochronology 688—689 754—755
Nucleosynthesis see “Thermonuclear reactions”
Nucleosynthesis, cosmological see “Big Bang nucleosynthesis”
Nyquist frequency 135—136
OB associations 633
Observer’s frame 263
Olbers paradox see “Halley — Olbers dark sky paradox”
Oort constants 656—657
Oort Law for Galactic rotation 655—658
Opacity, Kramers law 299
Opacity, line absorption 197—198
Opacity, photoionization 195
Opacity, Rosseland mean 190
Opacity, synchrotron 536 710—711
Opacity, thermal bremsstrahlung 193—194 243 299
Opacity, Thomson 299
Open clusters 633—635
Oppenheimer — Volkoff equation (also called Tolman — Oppenheimer — Volkoff equation) 390
Optical depth 179
Optical depth, scaling by wavelength-dependent opacity 227
Orbital motion, two-body problem 2—11
Orbital motion, two-body problem, in Schwarzschild metric 94
Orbital resonance see “Three-body problem”
Ortho-to-para (ortho:para) ratio for molecular hydrogen 490—491
Oscillator strength, defined 198
Ostriker — Peebles criterion 699—700
Outflows, thermal evaporation 62—64 249—250
Overshooting 305—306 369
Overstability 316
p-process 348 375—376 450 hydrogen
| Parallax 106—109
Parallax and proper motions 107—107
Parallax as basis of distance scale 740
Parallax, convergence point method 107—108
Parallax, Lutz — Keller bias 108—109
Parallax, statistical 108
Parceval’s theorem 162
Parker solution for stellar wind 249—250
Parsec, defined 107
Particle acceleration 528—531
Partition function 25—26 515
Period-luminosity relation 311—313 650 742—744
Periodogram 147
Perturbation theory 219—220 260—263
Phase space 20
Photodissociation 547—548
Photodissociation regions (PDR) 565—567
Photoionization 194—197 567—571
Photoionization, hydrogenic absorption coefficient 195
Planck mass 790
Planck radiation law 26 172
Planetary nebulae 378—380 750—751
plasma 46—49
Plasma frequency 47
Plasma, Debye — Hueckel model 356
Plasma, diffusion in 51—55
Plasma, screening in 48—49 355—356
Plasma, Stark effect 216—218
Plasma, thermal emission from 193 (see also “Thermal bremsstrahlung”)
Plasmon neutrino process 351—352
Point spread function (PSF) 134—135
Point spread function (psf), atmospheric turbulence and 142—145
Poisson equation 4 5 37—38
Poisson process see “Random processes Poisson”
Polarization, observations of interstellar 514—515
Polarization, Zeeman polarimetry 216
Polycyclic aromatic hydrocarbons (PAH) 513—514 552—554
Polytrope, defined 285—286
Polytrope, degenerate 298
Polytrope, Lane — Emden equation 294—299
Polytrope, limiting mass 297—298
Polytrope, polytropic indices 288 324
Polytrope, radiation-dominated 296—298
Polytrope, stability of 289—291
Polytropic equation of state 19
Population synthesis 675—677
Populous blue clusters 637
Power spectrum 142—144 162—163 624—627 828—830
Poynting — Robertson effect 508—509
Precession 7—11
Precession, orbital 10—11 94
Precession, rotational 8—10
Precursor, magnetic shocks 561—562
Precursor, radiative shock 563—564
Pressure broadening see “Stark effect” “Van
Pressure scale height 303
Pressure scale height for stellar hydrodynamics 644
Prior probability 151
Proper distance 79
Proper time 79
Proper volume 84
Protostar 364—366
Pulsars 394—401
Pulsation and virial theorem 59—60
Pulsation as analogy with a musical instrument 320—321
Pulsation as analogy with thermal cycle 315—316
Pulsation,  mechanism 316 374—375
Pulsation,  mechanism 316 318—319
Pulsation, linear pulsation equation 323—328
Pulsation, one-zone treatment 316—319
Pulsation, thermal pulsing on asymptotic giant branch 374—376
Q-parameter (pulsation) 312
Q-parameter (self-gravitation) see “Toomre criterion (Q)”
Q-value 331
Quasars see “Galaxies active
Quasiperiodic oscillations (QPO) 451—452
Quasistellar objects (QSO) see “Galaxies active
QUEUE 346—347
Quintessence see “Dark matter”
R-fronts see “H II regions as shocks”
r-process see “Neutron reactions”
Radiation pressure 245 286—288
Radiation pressure, equation of state 286—288
Radiation-dominated cosmology 780—781
Radiative damping 198
Radiative equilibrium 230—232 502—504
Radiative equilibrium and dust grains 242
Radiative flux, defined 177
Radiative flux, Eddington form, defined 178
Radiative flux, integrated, and Stefan — Boltzmann Law 178
Radiative temperature gradient 235 303
Radiative transfer equation in outflow 252—260 263—265
Radiative transfer equation, comoving frame 263—265 795—796
Radiative transfer equation, cosmological 795—796
Radiative transfer equation, diffusion approximation 190 300 440
Radiative transfer equation, discrete ordinates method 270—272
Radiative transfer equation, formal solution 182—184
Radiative transfer equation, gray atmosphere 232
Radiative transfer equation, invariant imbedding 265—268
Radiative transfer equation, limits of plane parallel approximation 186 238
Radiative transfer equation, moments of 176—179 180—182
Radiative transfer equation, plane parallel form 181 185—186
Radiative transfer equation, radiative equilibrium 230—232
Radiative transfer equation, scattering 183
Radiative transfer equation, spherical form 180—182 241—244
Radiative transfer equation, two-stream approximation 184
Radiative transfer equation, Wiener — Hopf solution 269—270
Radiative transition rates see “Transition probabilities”
Radio jets 713—715 728—730
Radionuclides 506 532—533 670—672 688—689 754—755
Random processes, Bayes’ theorem 150—151 163—165
Random processes, Gaussian 66 143—144 159 808 828
Random processes, Poisson 157—159 346—347 526—527 545—546
Random processes, queuing 346—347
Random processes, statistics 157—159
Random processes, stochastic differential equations 511—512
Random processes, stochastic sampling for time series 148—149
Rankine — Hugoniot relations 555—556
Rayleigh number 234 302—303
Rayleigh — Jeans approximation see “Blackbody radiation Rayleigh
Re-ionization epoch 823—826
Recombination 196—197
Recombination, definition of Case A and Case B 467
Recombination, lines 466—472
Reddening see “Extinction”
Redshift, cosmological 752—753 757 763—765
Redshift, effect on observable properties of galaxies 755—757
Redshift, gravitational 94
Redshift, surveys 808—811
Reflection nebulae 520—521
Resonance lines 476—477 492—495
Resonances, Lindblad resonances and galactic structure 662—668
Resonances, three-body problem 13—14
Reverberation mapping 706—707
Reynolds layer 493
Reynolds number, defined 44
Ricci tensor 88—89 760—762 766—767
Richardson — Lucy algorithm see “Algorithms Richardson
Riemann tensor 87—88
Roche lobe see “Roche radius”
Roche radius 6 418—420
Roche radius as limiting radius for components in close binaries 419—420
Roche radius as limiting radius for star clusters 64
Roche radius, analytical approximations 418—419
Rossby number 410
Rossiter — McLaughlin effect 436
Rotation measure 538
Rotation, gravity darkening 238—239
Rotation, line profile broadening 221—223
Rotation, Von Zeipel’s theorem 307—309
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