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astronomy & astrophysics (563) 563
astrophysics (401) 401
cosmology and extragalactic astrophysics (344) 344
agn feedback (334) 334
active galactic nuclei (325) 325
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feedback (120) 120
supermassive black-holes (112) 112
agn (104) 104
evolution (104) 104
methods: numerical (104) 104
physics - cosmology and nongalactic astrophysics (104) 104
astrophysics - high energy astrophysical phenomena (99) 99
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galaxy clusters (66) 66
intracluster medium (66) 66
cooling flows (63) 63
galaxies: formation (63) 63
galaxies: jets (63) 63
galaxy nuclei (63) 63
x-ray (61) 61
hydrodynamics (60) 60
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galaxies: clusters: intracluster medium (58) 58
physics (58) 58
black hole physics (54) 54
mass (52) 52
cosmology: theory (51) 51
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accretion disks (48) 48
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earth and planetary astrophysics (46) 46
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large-scale structure of universe (31) 31
universe (31) 31
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high-redshift (24) 24
accretion, accretion disks (23) 23
galaxies: kinematics and dynamics (23) 23
ism: jets and outflows (23) 23
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1. Full Text Relativistic jet feedback - III. Feedback on gas discs
by Mukherjee, Dipanjan and Bicknell, Geoffrey V and Wagner, Alexander Y and Sutherland, Ralph S and Silk, Joseph
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 10/2018, Volume 479, Issue 4, pp. 5544 - 5566
We study the interactions of a relativistic jet with a dense turbulent gaseous disc of radius similar to 2 kpc. We have performed a suite of simulations with... 
Galaxies: evolution | Hydrodynamics | Galaxies: highredshift | Galaxies: ism | Galaxies: jets | Methods: numerical | DRIVEN OUTFLOWS | SPIRAL GALAXY | galaxies: jets | STAR-FORMING GALAXIES | galaxies: evolution | GRAVITATIONALLY LENSED GALAXIES | hydrodynamics | INTERSTELLAR-MEDIUM | WIND-CLOUD INTERACTIONS | methods: numerical | BLACK-HOLES | AGN FEEDBACK | EQUATION-OF-STATE | ACTIVE GALACTIC NUCLEI | galaxies: ISM | ASTRONOMY & ASTROPHYSICS | galaxies: highredshift
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2. Full Text Quasar feedback revealed by giant molecular outflows
by Feruglio, C and Maiolino, R and Piconcelli, E and Menci, N and Aussel, H and Lamastra, A and Fiore, F
Astronomy and Astrophysics, ISSN 0004-6361, 08/2010, Volume 518, Issue 13, p. L155
In the standard scenario for galaxy evolution young star-forming galaxies transform into red bulge-dominated spheroids, where star formation has been quenched.... 
Galaxies: evolution | Galaxies: active | Galaxies: individual: Mrk 231 | Quasars: general | quasars: general | galaxies: evolution | STAR-FORMATION | HOST GALAXIES | SIMILAR-TO 1 | BLACK-HOLES | AGN FEEDBACK | galaxies: individual: Mrk 231 | ACTIVE GALACTIC NUCLEI | galaxies: active | ASTRONOMY & ASTROPHYSICS | SDSS J0318-0600 | STELLAR OBJECTS | MARKARIAN 231 | ULTRALUMINOUS INFRARED GALAXIES | Physics - Cosmology and Nongalactic Astrophysics
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3. Full Text Toward a comprehensive model for feedback by active galactic nuclei: New insights from M87 observations by LOFAR, FERMI, and H.E.S.S
by Pfrommer, Christoph
Astrophysical Journal, ISSN 0004-637X, 12/2013, Volume 779, Issue 1, pp. 10 - 18
Feedback by active galactic nuclei (AGNs) appears to be critical in balancing radiative cooling of the low-entropy gas at the centers of galaxy clusters and in... 
gamma rays: galaxies: clusters | galaxies: individual (M87) | cosmic rays | galaxies: active | galaxies: clusters: intracluster medium | radio continuum: galaxies | MAGNETIC-FIELDS | THERMAL-INSTABILITY | PERSEUS GALAXY CLUSTER | AGN FEEDBACK | GAMMA-RAY EMISSION | INTRACLUSTER MEDIUM | ASTRONOMY & ASTROPHYSICS | VIRGO CLUSTER | X-RAY | COSMIC-RAYS | COOLING-FLOW CLUSTERS | Active galactic nuclei | Halos | Cooling | Heating | Feedback | LOFAR | Mathematical models | Radio | X RADIATION | INSTABILITY | ELECTRONS | GALAXY CLUSTERS | RADIATIVE COOLING | GAMMA RADIATION | KEV RANGE | INTERACTIONS | PROTONS | COSMIC RADIATION | ALFVEN WAVES | FORECASTING | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | THERMAL EQUILIBRIUM | SCALING | STARS | EMISSION | SPECTRA | GALAXY NUCLEI
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4. Full Text Cosmic-Ray Feedback Heating of the Intracluster Medium
by Ruszkowski, Mateusz and Yang, H.-Y. Karen and Reynolds, Christopher S
Astrophysical Journal, ISSN 0004-637X, 07/2017, Volume 844, Issue 1, p. 13
Active galactic nuclei (AGNs) play a central role in solving the decades-old cooling-flow problem. Although there is consensus that AGNs provide the energy to... 
MAGNETOHYDRODYNAMIC SIMULATIONS | GALAXY CLUSTERS | PERSEUS CLUSTER | galaxies: clusters: intracluster medium | COOLING FLOWS | AGN FEEDBACK | RADIO BUBBLES | cosmic rays | ACTIVE GALACTIC NUCLEI | galaxies: active | ASTRONOMY & ASTROPHYSICS | STAGGERED MESH SCHEME | VISCOUS DISSIPATION | ANISOTROPIC THERMAL CONDUCTION | Physics - High Energy Astrophysical Phenomena | DISPERSIONS | INSTABILITY | THERMALIZATION | LIMITING VALUES | SIMULATION | THREE-DIMENSIONAL CALCULATIONS | ATMOSPHERES | COSMIC RADIATION | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | AVAILABILITY | STARS | GALAXIES | HADRONS | FEEDBACK | GALAXY NUCLEI
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5. Full Text Black hole feedback in the luminous quasar PDS 456
by Nardini, E and Reeves, J.N and Gofford, J and Harrison, F.A and Risaliti, G and Braito, V and Costa, M.T and Matzeu, G.A and Walton, D.J and Behar, E and Boggs, S.E and Christensen, F.E and Craig, W.W and Hailey, C.J and Matt, G and Miller, J.M and O'Brien, P.T and Stern, D and Turner, T.J and Ward, M.J
Science, ISSN 0036-8075, 02/2015, Volume 347, Issue 6224, pp. 860 - 863
The evolution of galaxies is connected to the growth of supermassive black holes in their centers. During the quasar phase, a huge luminosity is released as... 
WIND | LOCATION | ABSORBER | OUTFLOWS | RADIO-QUIET AGNS | SIGMA RELATION | MULTIDISCIPLINARY SCIENCES | HOST GALAXIES | Quasars | Observations | Black holes (Astronomy) | Luminosity | Evolutionary biology | Black holes | Stars & galaxies | Galaxies | Feedback | Astronomical models | Wind power generation | Black holes (astronomy) | Outflow | Signatures | Physics - High Energy Astrophysical Phenomena
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6. Full Text The impact of feedback on cosmological gas accretion
by Nelson, Dylan and Genel, Shy and Vogelsberger, Mark and Springel, Volker and Sijacki, Debora and Torrey, Paul and Hernquist, Lars
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2015, Volume 448, Issue 1, pp. 59 - 74
We investigate how the way galaxies acquire their gas across cosmic time in cosmological hydrodynamic simulations is modified by a comprehensive physical model... 
Galaxies: evolution | Cosmology: theory | Galaxies: haloes | Galaxies: formation | Methods: numerical | galaxies: evolution | STELLAR FEEDBACK | ILLUSTRIS PROJECT | STAR-FORMATION | methods: numerical | SUPERMASSIVE BLACK-HOLES | cosmology: theory | AGN FEEDBACK | galaxies: formation | ACTIVE GALACTIC NUCLEI | ASTRONOMY & ASTROPHYSICS | MOVING-MESH COSMOLOGY | COLD FLOWS | GALAXY FORMATION | DISC FORMATION | galaxies: haloes
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7. Full Text Momentum Driving: Which Physical Processes Dominate Active Galactic Nucleus Feedback?
by Ostriker, Jeremiah P and Choi, Ena and Ciotti, Luca and Novak, Gregory S and Proga, Daniel
The Astrophysical Journal, ISSN 0004-637X, 10/2010, Volume 722, Issue 1, pp. 642 - 652
The deposition of mechanical feedback from a supermassive black hole (SMBH) in an active galactic nucleus into the surrounding galaxy occurs via broad-line... 
Galaxies: nuclei | Galaxies: active | Galaxies: starburst | Accretion, accretion disks | Quasars: general | Black hole physics | galaxies: starburst | quasars: general | MASSIVE BLACK-HOLES | ELLIPTIC GALAXIES | accretion, accretion disks | SLOW JETS | MECHANICAL FEEDBACK | AGN FEEDBACK | DRIVEN DISK WINDS | ACCRETION-DISK | QUASARS | black hole physics | galaxies: active | ASTRONOMY & ASTROPHYSICS | galaxies: nuclei | RADIATION PRESSURE | COSMIC-RAYS | COSMIC RADIO SOURCES | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | GALAXIES | SIMULATION | TWO-DIMENSIONAL CALCULATIONS | ACCRETION DISKS | BLACK HOLES | GALAXY NUCLEI
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8. Full Text Simulating galaxy formation with black hole driven thermal and kinetic feedback
by Weinberger, Rainer and Springel, Volker and Hernquist, Lars and Pillepich, Annalisa and Marinacci, Federico and Pakmor, Rüdiger and Nelson, Dylan and Genel, Shy and Vogelsberger, Mark and Naiman, Jill and Torrey, Paul
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2017, Volume 465, Issue 3, pp. 3291 - 3308
The inefficiency of star formation in massive elliptical galaxies is widely believed to be caused by the interactions of an active galactic nucleus (AGN) with... 
Galaxies: clusters: general | Galaxies: evolution | Cosmology: theory | Galaxies: formation | Black hole physics | Methods: numerical | JET-INFLATED BUBBLES | galaxies: clusters: general | STAR-FORMING GALAXIES | SIMILAR-TO 2 | methods: numerical | SMOOTHED PARTICLE HYDRODYNAMICS | HIGH-REDSHIFT GALAXIES | cosmology: theory | galaxies: formation | black hole physics | ACTIVE GALACTIC NUCLEI | INTRACLUSTER MEDIUM | ASTRONOMY & ASTROPHYSICS | MOVING-MESH COSMOLOGY | COOL-CORE CLUSTERS | galaxies:evolution | MECHANICAL AGN FEEDBACK | Physics - Astrophysics of Galaxies
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9. Full Text Feedback from active galactic nuclei: Energy- versus momentum-driving
by Costa, Tiago and Sijacki, Debora and Haehnelt, Martin G
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2014, Volume 444, Issue 3, pp. 2355 - 2376
We employ hydrodynamical simulations using the moving-mesh code AREPO to investigate the role of energy and momentum input from active galactic nuclei (AGN) in... 
Methods: Numerical | Cosmology: Theory | Black hole physics | RADIO-QUIET AGNS | methods: numerical | SUPERMASSIVE BLACK-HOLES | COSMOLOGICAL SIMULATIONS | cosmology: theory | QUASAR FEEDBACK | ULTRA-FAST OUTFLOWS | black hole physics | SIMILAR-TO 6 | M-BH-SIGMA | BRIGHTEST CLUSTER GALAXIES | ASTRONOMY & ASTROPHYSICS | SHELL ABSORPTION-LINES | MASSIVE MOLECULAR OUTFLOWS
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10. Full Text NIHAO - XXII. Introducing black hole formation, accretion, and feedback into the NIHAO simulation suite
by Blank, M and Maccio, AV and Dutton, AA and Obreja, A
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 08/2019, Volume 487, Issue 4, pp. 5476 - 5489
We introduce algorithms for black hole physics, i.e. black hole formation, accretion, and feedback, into the Numerical Investigation of a Hundred Astrophysical... 
quasars: general | ANGULAR-MOMENTUM | galaxies: evolution | ILLUSTRIS PROJECT | DARK-MATTER HALOES | STAR-FORMATION | INTERSTELLAR MATTER | methods: numerical | COSMOLOGICAL SIMULATIONS | AGN FEEDBACK | galaxies: formation | EVOLUTION | ACTIVE GALACTIC NUCLEI | galaxies: active | ASTRONOMY & ASTROPHYSICS | GALAXY FORMATION | galaxies: nuclei | Physics - Astrophysics of Galaxies
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11. Full Text Active galactic nucleus feedback in an isolated elliptical galaxy: The effect of strong radiative feedback in the kinetic mode
by Gan, Zhaoming and Yuan, Feng and Ostriker, Jeremiah P and Ciotti, Luca and Novak, Gregory S
Astrophysical Journal, ISSN 0004-637X, 07/2014, Volume 789, Issue 2, pp. 150 - 14
Based on two-dimensional high-resolution hydrodynamic numerical simulation, we study the mechanical and radiative feedback effects from the central active... 
galaxies: elliptical and lenticular, cD | black hole physics | galaxies: nuclei | accretion, accretion disks | galaxies: active | galaxies: evolution | OBSERVATIONAL EVIDENCE | NEARBY GALAXIES | ADVECTION-DOMINATED ACCRETION | VELOCITY DISPERSION | HOST GALAXIES | MASS OUTFLOWS | COOLING FLOWS | SPECTRAL ENERGY-DISTRIBUTIONS | ASTRONOMY & ASTROPHYSICS | MECHANICAL AGN FEEDBACK | CENTRAL BLACK-HOLES | Active galactic nuclei | Accretion | Computer simulation | Heating | Feedback | Astronomical models | Luminosity | Mathematical models | LUMINOSITY | X RADIATION | MECHANICAL EFFICIENCY | RESOLUTION | TWO-DIMENSIONAL CALCULATIONS | ACCRETION DISKS | BLACK HOLES | COMPUTERIZED SIMULATION | EVOLUTION | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | GALAXIES | EMISSION | SPECTRA | FEEDBACK | GALAXY NUCLEI
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12. Full Text Direct detection of quasar feedback via the Sunyaev-Zeldovich effect
by Lacy, M and Mason, B and Sarazin, C and Chatterjee, S and Nyland, K and Kimball, A and Rocha, G and Rowe, B and Surace, J
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 02/2019, Volume 483, Issue 1, pp. L22 - L27
The nature and energetics of feedback from thermal winds in quasars can be constrained via observations of the Sunyaev-Zeldovich Effect ( SZE) induced by the... 
quasars: individual HE 0515-4414 | SKY | quasars: general | ACTIVE GALACTIC NUCLEI | galaxies: evolution | ASTRONOMY & ASTROPHYSICS | GAS | DRIVEN | BLACK-HOLES | AGN FEEDBACK
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13. Full Text Self-regulated growth of supermassive black holes by a dual jet-heating active galactic nucleus feedback mechanism: methods, tests and implications for cosmological simulations
by Dubois, Yohan and Devriendt, Julien and Slyz, Adrianne and Teyssier, Romain
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2012, Volume 420, Issue 3, pp. 2662 - 2683
We develop a subgrid model for the growth of supermassive black holes (BHs) and their associated active galactic nucleus (AGN) feedback in hydrodynamical... 
quasars: general | galaxies: jets | methods: numerical | galaxies: active | galaxies: evolution | Galaxies: evolution | Galaxies: active | Quasars: general | Galaxies: jets | Methods: numerical | MAGNETOHYDRODYNAMIC SIMULATIONS | BULGE MASS RELATION | VELOCITY DISPERSION | STAR-FORMING GALAXIES | ELLIPTIC GALAXIES | HOST GALAXIES | AGN FEEDBACK | DIGITAL SKY SURVEY | COSMIC EVOLUTION | ASTRONOMY & ASTROPHYSICS | X-RAY CAVITIES | Cosmology | Astrophysics | Simulation | Black holes | Stars & galaxies | Computer simulation | Galaxies | Feedback | Black holes (astronomy) | Outflow | Mathematical models | Nuclei | Deposition
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