The formation of dusty cold gas filaments from galaxy cluster simulations
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B. McNamara | M. McDonald | T. Bogdanović | Y. Qiu | Yuan Li
[1] E. Quataert,et al. The Fate of Asymptotic Giant Branch Winds in Massive Galaxies and the Intracluster Medium , 2019, The Astrophysical Journal.
[2] E. Dwek,et al. Dust Formation in AGN Winds , 2019, The Astrophysical Journal.
[3] Y. Dubois,et al. Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback , 2019, Astronomy & Astrophysics.
[4] B. Benson,et al. Anatomy of a Cooling Flow: The Feedback Response to Pure Cooling in the Core of the Phoenix Cluster , 2019, The Astrophysical Journal.
[5] A. Edge,et al. Driving massive molecular gas flows in central cluster galaxies with AGN feedback , 2019, Monthly Notices of the Royal Astronomical Society.
[6] M. McDonald,et al. Using Hα Filaments to Probe Active Galactic Nuclei Feedback in Galaxy Clusters , 2019, The Astrophysical Journal.
[7] J. Wise,et al. The Interplay of Kinetic and Radiative Feedback in Galaxy Clusters , 2018, The Astrophysical Journal.
[8] Devin W. Silvia,et al. ENZO: AN ADAPTIVE MESH REFINEMENT CODE FOR ASTROPHYSICS , 2013, J. Open Source Softw..
[9] P. Nulsen,et al. A Universal Entropy Profile for the Hot Atmospheres of Galaxies and Clusters within R2500 , 2018, The Astrophysical Journal.
[10] A. Edge,et al. Revealing the velocity structure of the filamentary nebula in NGC 1275 in its entirety. , 2018, 1802.00031.
[11] A. Edge,et al. The Onset of Thermally Unstable Cooling from the Hot Atmospheres of Giant Galaxies in Clusters: Constraints on Feedback Models , 2017, 1704.00011.
[12] E. Quataert,et al. Entrainment in trouble: cool cloud acceleration and destruction in hot supernova-driven galactic winds , 2015, 1507.01951.
[13] B. Benson,et al. Alma Observations of Massive Molecular Gas Filaments Encasing Radio Bubbles in the Phoenix Cluster , 2016, 1611.00017.
[14] C. Conselice,et al. HST imaging of the dusty filaments and nucleus swirl in NGC4696 at the centre of the Centaurus Cluster , 2016, 1606.02436.
[15] M. Donahue,et al. Cold, clumpy accretion onto an active supermassive black hole , 2016, Nature.
[16] A. Edge,et al. A MECHANISM FOR STIMULATING AGN FEEDBACK BY LIFTING GAS IN MASSIVE GALAXIES , 2016, 1604.04629.
[17] B. Benson,et al. DEEP CHANDRA, HST-COS, AND MEGACAM OBSERVATIONS OF THE PHOENIX CLUSTER: EXTREME STAR FORMATION AND AGN FEEDBACK ON HUNDRED KILOPARSEC SCALES , 2015, 1508.05941.
[18] B. McNamara,et al. Hot Outflows in Galaxy Clusters , 2015, 1507.05973.
[19] A. Edge,et al. Effects of the variability of the nucleus of NGC1275 on X-ray observations of the surrounding intracluster medium , 2015, 1505.03754.
[20] A. Babul,et al. COOL CORE CYCLES: COLD GAS AND AGN JET FEEDBACK IN CLUSTER CORES , 2015, 1504.02215.
[21] M. Donahue,et al. COOLING, AGN FEEDBACK, AND STAR FORMATION IN SIMULATED COOL-CORE GALAXY CLUSTERS , 2015, 1503.02660.
[22] M. Donahue,et al. Regulation of star formation in giant galaxies by precipitation, feedback and conduction , 2014, Nature.
[23] A. Fabian,et al. A volume-limited sample of X-ray galaxy groups and clusters – I. Radial entropy and cooling time profiles , 2013, 1312.0798.
[24] Adrian T. Lee,et al. A massive, cooling-flow-induced starburst in the core of a luminous cluster of galaxies , 2012, Nature.
[25] M. Donahue,et al. Herschel observations of extended atomic gas in the core of the Perseus cluster , 2012, 1208.1730.
[26] Andrew C. Fabian,et al. Observational Evidence of Active Galactic Nuclei Feedback , 2012 .
[27] P. Sharma,et al. CAUSE AND EFFECT OF FEEDBACK: MULTIPHASE GAS IN CLUSTER CORES HEATED BY AGN JETS , 2011, 1110.6063.
[28] S. Veilleux,et al. OPTICAL SPECTROSCOPY OF Hα FILAMENTS IN COOL CORE CLUSTERS: KINEMATICS, REDDENING, AND SOURCES OF IONIZATION , 2011, 1111.0006.
[29] M. Donahue,et al. Herschel observations of the Centaurus cluster – the dynamics of cold gas in a cool core , 2011, 1108.2757.
[30] Usa,et al. The Energy Source of the Filaments Around the Giant Galaxy NGC 1275 , 2011, 1105.1735.
[31] M. Donahue,et al. POLYCYCLIC AROMATIC HYDROCARBONS, IONIZED GAS, AND MOLECULAR HYDROGEN IN BRIGHTEST CLUSTER GALAXIES OF COOL-CORE CLUSTERS OF GALAXIES , 2011, 1103.1410.
[32] T. Abel,et al. enzo+moray: radiation hydrodynamics adaptive mesh refinement simulations with adaptive ray tracing , 2010, 1012.2865.
[33] S. Veilleux,et al. ON THE ORIGIN OF THE EXTENDED Hα FILAMENTS IN COOLING FLOW CLUSTERS , 2010, 1008.0392.
[34] M. Bremer,et al. The distribution and condition of the warm molecular gas in Abell 2597 and Sersic 159-03 , 2010, 1002.3297.
[35] C. Conselice,et al. Magnetic support of the optical emission line filaments in NGC 1275 , 2008, Nature.
[36] C. Crawford,et al. Ionized nebulae surrounding brightest cluster galaxies , 2007, 0706.0661.
[37] M. Hudson,et al. Line emission in the brightest cluster galaxies of the NOAO Fundamental Plane and Sloan Digital Sky Surveys , 2007, 0704.3242.
[38] G. Ferland,et al. Discovery of Atomic and Molecular Mid-Infrared Emission Lines in Off-Nuclear Regions of NGC 1275 and NGC 4696 with the Spitzer Space Telescope , 2007, astro-ph/0702431.
[39] F. Brighenti,et al. Heating Cooling Flows with Weak Shock Waves , 2005, astro-ph/0511151.
[40] G. Bryan,et al. Structure Formation , 2005 .
[41] M. Bremer,et al. HII and H2 in the envelopes of cooling flow central galaxies , 2005, astro-ph/0504413.
[42] I. Cambridge,et al. The nature of the molecular gas system in the core of NGC 1275 , 2005, astro-ph/0502537.
[43] C. Carilli,et al. The heating of gas in a galaxy cluster by X-ray cavities and large-scale shock fronts , 2005, Nature.
[44] P. Nulsen,et al. ACCEPTED FOR PUBLICATION IN THE ASTROPHYSICAL JOURNAL Preprint typeset using LATEX style emulateapj v. 4/12/04 A SYSTEMATIC STUDY OF RADIO-INDUCED X-RAY CAVITIES IN CLUSTERS, GROUPS, AND GALAXIES , 2004 .
[45] W. Forman,et al. XMM—Newton observations of the Perseus cluster — II. Evidence for gas motions in the core , 2003, astro-ph/0309427.
[46] F. Combes,et al. Cold molecular gas in cooling flow clusters of galaxies , 2003, astro-ph/0309304.
[47] A. Edge,et al. Resolving Molecular Gas in the Central Galaxies of Cooling Flow Clusters , 2003 .
[48] C. Conselice,et al. On the Nature of the NGC 1275 System , 2001, astro-ph/0108019.
[49] A. Edge. The detection of molecular gas in the central galaxies of cooling flow clusters , 2001, astro-ph/0106225.
[50] M. Bremer,et al. Infrared spectra of cooling flow galaxies , 2000, astro-ph/0009418.
[51] Institute for Astronomy,et al. The ROSAT Brightest Cluster Sample — III. Optical spectra of the central cluster galaxies , 1999, astro-ph/9903057.
[52] G. Lake,et al. The Structure of Cold Dark Matter Halos , 1998 .
[53] H. Nørgaard-Nielsen,et al. Interstellar matter in Shapley-Ames elliptical galaxies. II. The distribution of dust and ionized gas , 1994 .
[54] W. Sparks,et al. Imaging observations of gas and dust in NGC 4696 and implications for cooling flow models , 1989 .
[55] Patrick J. McCarthy,et al. Dynamical, physical, and chemical properties of emission-line nebulae in cooling flows , 1989 .
[56] Raymond E. White,et al. Steady state cooling flow models for normal elliptical galaxies , 1987 .
[57] A. Fabian,et al. The optical spectra of central galaxies in southern clusters: evidence for star formation , 1987 .
[58] L. Cowie,et al. Long-slit spectroscopy of gas in the cores of X-ray luminous clusters , 1985 .
[59] E. Salpeter,et al. On the physics of dust grains in hot gas. , 1979 .