The heating of gas in a galaxy cluster by X-ray cavities and large-scale shock fronts

[1]  P. Nulsen,et al.  The Cluster-Scale AGN Outburst in Hydra A , 2004, astro-ph/0408315.

[2]  J. Brinchmann,et al.  Present-Day Growth of Black Holes and Bulges: The Sloan Digital Sky Survey Perspective , 2004, astro-ph/0406218.

[3]  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 .

[4]  R. Kraft,et al.  Reflections of AGN Outbursts in the Gaseous Atmosphere of M87 , 2004 .

[5]  C. S. Crawford,et al.  A deep Chandra observation of the Perseus cluster: shocks and ripples , 2003, astro-ph/0306036.

[6]  J. Jernigan,et al.  High-Resolution X-Ray Spectroscopic Constraints on Cooling-Flow Models for Clusters of Galaxies , 2002, astro-ph/0210662.

[7]  W. Orman,et al.  Reflections of Agn Outbursts in the Gaseous Atmosphere of M87 , 2003 .

[8]  R. Sunyaev,et al.  Cooling flows as a calorimeter of active galactic nucleus mechanical power , 2002 .

[9]  S. Colgate,et al.  Magnetic Energy of the Intergalactic Medium from Galactic Black Holes , 2001, astro-ph/0106281.

[10]  A. Edge.  The detection of molecular gas in the central galaxies of cooling flow clusters , 2001, astro-ph/0106225.

[11]  A. Loeb,et al.  Intergalactic Magnetic Fields from Quasar Outflows , 2001, astro-ph/0102076.

[12]  A. Fabian,et al.  On the soft X-ray spectrum of cooling flows , 2000, astro-ph/0010509.

[13]  Raymond E. White,et al.  A Moderate Cluster Cooling Flow Model , 2000, astro-ph/0009173.

[14]  U. Toronto,et al.  A New Radio-X-Ray Probe of Galaxy Cluster Magnetic Fields , 2000, astro-ph/0011281.

[15]  H.Bohringer,et al.  Evolution of Buoyant Bubbles in M87 , 2000, astro-ph/0008215.

[16]  Ralf Bender,et al.  A Relationship between Nuclear Black Hole Mass and Galaxy Velocity Dispersion , 2000, astro-ph/0006289.

[17]  D. Merritt,et al.  A Fundamental Relation between Supermassive Black Holes and Their Host Galaxies , 2000, astro-ph/0006053.

[18]  D. Harris,et al.  Chandra X-Ray Observations of the Hydra A Cluster: An Interaction between the Radio Source and the X-Ray-emitting Gas , 2000, The Astrophysical journal.

[19]  Non‐gravitational heating in the hierarchical formation of X‐ray clusters , 1999, astro-ph/9907112.

[20]  Maxim Markevitch,et al.  The LX-T Relation and Temperature Function for Nearby Clusters Revisited , 1998, astro-ph/9802059.

[21]  C. Reynolds,et al.  X-Ray Signatures of Evolving Radio Galaxies , 1998, astro-ph/9801268.

[22]  M. Dopita,et al.  Unification of the Radio and Optical Properties of Gigahertz Peak Spectrum and Compact Steep-Spectrum Radio Sources , 1997 .

[23]  M. Donahue,et al.  ROSAT observations of distant clusters of galaxies , 1995 .

[24]  E. Greisen,et al.  The NRAO VLA Sky Survey , 1996 .

[25]  D. Young.  On the relation between Fanaroff-Riley types I and II radio galaxies , 1993 .

[26]  M. Donahue,et al.  Distant cooling flows , 1992 .

[27]  Isabella M. Gioia,et al.  The Einstein Observatory Extended Medium-Sensitivity Survey. II - The optical identifications , 1991 .

[28]  B. McNamara,et al.  Star formation in cooling flows in clusters of galaxies , 1989 .

[29]  A. Fabian,et al.  Cooling flows in clusters of galaxies , 1984, Nature.

[30]  P. A. G. Scheuer,et al.  Models of Extragalactic Radio Sources with a Continuous Energy Supply from a Central Object , 1974 .