Авторизация
Поиск по указателям
Alloin D., Johnson R., Lira P. — Physics of Active Galactic Nuclei at all Scales
Обсудите книгу на научном форуме
Нашли опечатку? Выделите ее мышкой и нажмите Ctrl+Enter
Название: Physics of Active Galactic Nuclei at all Scales
Авторы: Alloin D., Johnson R., Lira P.
Аннотация: The source of energy in Active Galactic Nuclei is commonly accepted to be gravitational energy released through accretion of matter onto a supermassive black hole. Since the discovery of the first radio galaxies and quasars in the early sixties tremendous progress has been made in unveiling, analyzing and modelling the different components in AGN: the accretion disk, the jets of relativistic particles, the X-ray absorber close to the central engine, the "torus" which funnels the ionizing radiation, the surrounding clouds of dense material in the broad-line region and narrow-line region, the cool molecular and dusty material around the torus, as well as jet-induced effects on larger scales. Yet, it remains to incorporate all these components and physical processes in a self-consistent AGN model which would take into account, and predict, all the facets of observed AGN activity. Besides discussing the elements of this "Unified Model of AGN" this book also addresses the still not entirely understood link of an AGN with its host galaxy and also the related question of the birth and growth of massive black holes in the Universe, which is of prime interest for cosmology.
Язык:
Рубрика: Физика /
Статус предметного указателя: Готов указатель с номерами страниц
ed2k: ed2k stats
Год издания: 2006
Количество страниц: 234
Добавлена в каталог: 04.02.2010
Операции: Положить на полку |
Скопировать ссылку для форума | Скопировать ID
Предметный указатель
Absorption, broad absorption lines 30 31 221
Absorption, free-free 109
Acceleration of particles 62
Accretion disk 4—10 35
Accretion disk, ADAF 11
Accretion disk, corona 10
Accretion disk, geometry 4 8 10
Accretion disk, spectrum 9
Accretion disk, structure 4 8
Accretion disk, temperature 6 7
Accretion disk, viscosity 7
Accretion, efficiency 3 147
Accretion, flow 143
Accretion, spherical, Bondi 3 101
Active galactic nuclei (AGN), classification 1 52 216
Active galactic nuclei (AGN), density of 201
Active galactic nuclei (AGN), environmental impact 222
Active galactic nuclei (AGN), evolution 196
Active galactic nuclei (AGN), unified model 25 62 101 102 111 114
Angular momentum, release 174
Angular momentum, specific 149 174
Auger ionization 14
Baldwin relation 80
Bars, large-scale 151 160
Bars, nuclear 169
BL Lac objects 63 67
Black holes, evidence for 77 185 211 212
Black holes, formation 219 223
Black holes, mass 89 144 213
Black holes, mass density 151
Black holes, mass-sigma relation 146 213 219 224
Black holes, properties 1 212
Blazars 70
Bloated stars 19 33 92
Broad line region (BLR) 25 77
Broad line region (BLR), model 91
Broad line region (BLR), size 86
Cen A 54 65—67
Charge exchange 14
Clumpiness 115
CO observations 104 117
Collisional, excitation 16
Collisional, ionization 14 15
confinement 19 25 26 64
Continuum emission 17
Cooling flow 222
Cygnus A 64
Dielectronic recombination 14
Doppler factor 47
Dust in BLR/NLR 27
Dust in torus 102 104 109 114 115
Dust, silicate feature 114
Dust, sublimation 27 103 115
Dust, Temperature 103 115
Dynamical friction 150 174
Eddington, accretion rate 3
Eddington, luminosity 2 81
Eddington, time 3
Emission lines, coronal 27
Emission lines, profiles BLR/NLR 26 92—95
Equipartition 57 59
Faraday rotation 60 67
Faranov — Riley classes (FRI, FRII) 52 54
Fluorescence (line and continuum) 18 19
Force multiplier 23
Free-free absorption 109
Fueling, growth 2 101 143 148 151 160 169
Galaxy formation 214 217
Gaunt factor 44
H2 emission 104
HI absorption 106 108
Highly ionized gas (HIG) 30
Host galaxy 154 160
Hot intercloud medium (HIM) 19 26
Hot spots 53
Hydrostatic equilibrium 48
identifications 191 217
Inflow 151 160
Infrared emission 113
Intergalactic medium (IGM) 48 64 223
Inverse Compton scattering 42 47 61 69
Ionization, cone 102
Ionization, parameter 17 78
Isothermal gas 49
Jets, acceleration 62
Jets, composition 59
Jets, confinement 64
Jets, high power 52
Jets, interaction with external medium 48
Jets, low power 54
Jets, magnetic fields 56 63 67
Jets, speed 52 56 61
K-shell lines 19 102
Lindblad resonances 160
Line cooling 15
Lorentz factor 40 42 46 69
Luminosity function 197 212 216 219
M87 56
Mach number 52
Masers 110
Mechanical heating 16
mergers 149 156 159
Molecular gas 104 106
Narrow line region (NLR) 26 78 102
NGC 1068 104 113 118
Outflows, winds 19 22 36 94 95 175 220 222 225
Photoionization 13 78
Polarization 67 69
Radiation, pressure 2 22 24
Radiation, self-Compton (SSC) 43 47 58
Radiation, synchrotron 40 56 70
Radiation, thermal 44
Radiative transfer 16 114
Radio galaxies, radio sources 52 70
Rankine — Hugoniot conditions 54
Recombination 13 14
Relativistic beaming 47 58
Reverberation mapping 27 81
Sag A* 212
Scattering 10
SCUBA sources 199 217
Shocks 52 150
Spectral energy distribution (SED) 11 113 117
Stability curve 20
Starburst 16 33 152 156 160 165 171 193
Superluminal motion 46
Surveys 185 198
Temperature, dust 103 115
Temperature, electron 78
Thermal, balance 15
Thermal, radiation 44
Tidal/gravitational torque 5 150 151
Torus 33 115 116
UV absorber 25
Variability of BLR 81
Variability, time delay 82
Variability, velocity-delay map 83
Viscosity, stress 7
Viscosity, torque 150 175
Warm absorber 30
X-ray, absorption 30 102 106
X-ray, background (XRB) 194 196
X-ray, Compton thick absorption 196
X-ray, emission 198 200
X-ray, space missions 185 206
X-ray, variability 113 117
Реклама