EPISODIC RANDOM ACCRETION AND THE COSMOLOGICAL EVOLUTION OF SUPERMASSIVE BLACK HOLE SPINS
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Shu Zhang | Andrew King | Luis C. Ho | Chen Hu | Rüdiger Staubert | Jian-Min Wang | Yan-Rong Li | Yan-Mei Chen | Alessandro Marconi | C. T. Yan | L. Ho | A. King | Chen Hu | A. Marconi | Yan-Rong Li | R. Staubert | Shu Zhang | Jian-Min Wang | Changshuo Yan | Yan-Mei Chen | A. King
[1] F. Walter,et al. The Recent Star Formation Histories of M81 Group Dwarf Irregular Galaxies , 2008, 0809.5059.
[2] Cosmological Evolution of the Duty Cycle of Quasars , 2006, astro-ph/0606704.
[3] J. Lasota,et al. Radio Loudness of Active Galactic Nuclei: Observational Facts and Theoretical Implications , 2006, astro-ph/0604095.
[4] S. Tremaine,et al. Observational constraints on growth of massive black holes , 2002, astro-ph/0203082.
[5] Black Hole Mass and Spin Coevolution by Mergers , 2002, astro-ph/0208484.
[6] G. Richards,et al. Mass Functions of the Active Black Holes in Distant Quasars from the Sloan Digital Sky Survey Data Release 3 , 2007, 0801.0243.
[7] K. Thorne. Disk-Accretion onto a Black Hole. II. Evolution of the Hole , 1974 .
[8] T. D. Matteo,et al. Energy input from quasars regulates the growth and activity of black holes and their host galaxies , 2005, Nature.
[9] Ralf Bender,et al. The Demography of massive dark objects in galaxy centers , 1997, astro-ph/9708072.
[10] A. Mazure,et al. The VVDS type-1 AGN sample: the faint end of the luminosity function , 2007, 0704.1660.
[11] Henry C. Ferguson,et al. The Evolution of the Optical and Near-Infrared Galaxy Luminosity Functions and Luminosity Densities to z ~ 2 , 2005 .
[12] John Kormendy,et al. Inward Bound—The Search for Supermassive Black Holes in Galactic Nuclei , 1995 .
[13] Marta Volonteri,et al. Cosmological Black Hole Spin Evolution by Mergers and Accretion , 2008, 0802.0025.
[14] On the black hole–bulge mass relation in active and inactive galaxies , 2001, astro-ph/0108417.
[15] F. Schweitzer,et al. Galaxies : interactions and induced star formation , 1998 .
[16] L. Ho. The CO Tully-Fisher Relation and Implications for the Host Galaxies of High-Redshift Quasars , 2007, 0707.3436.
[17] E. Turner,et al. Remnants of the quasars. , 1992 .
[18] Yue Shen,et al. Modeling Porous Dust Grains with Ballistic Aggregates. I. Geometry and Optical Properties , 2008, 0801.1996.
[19] Laura Ferrarese David Merritt. A Fundamental Relation Between Supermassive Black Holes and Their Host Galaxies , 2000, astro-ph/0006053.
[20] Volker Springel,et al. The Many lives of AGN: Cooling flows, black holes and the luminosities and colours of galaxies , 2006, astro-ph/0602065.
[21] Ralf Bender,et al. A Relationship between Nuclear Black Hole Mass and Galaxy Velocity Dispersion , 2000, astro-ph/0006289.
[22] Ralf Bender,et al. THE SLOPE OF THE BLACK HOLE MASS VERSUS VELOCITY DISPERSION CORRELATION , 2002, astro-ph/0203468.
[23] R. Blandford,et al. Quasar evolution and the growth of black holes , 1992 .
[24] Xiaohui Fan,et al. DETERMINING QUASAR BLACK HOLE MASS FUNCTIONS FROM THEIR BROAD EMISSION LINES: APPLICATION TO THE BRIGHT QUASAR SURVEY , 2008, 0811.2001.
[25] Andrzej Soƚtan,et al. Masses of quasars , 1982 .
[26] Andrew M. Hopkins,et al. On the Normalization of the Cosmic Star Formation History , 2006, astro-ph/0601463.
[27] Marek Sikora,et al. Black Hole Spin and Galactic Morphology , 2007, 0706.3900.
[28] A. Szalay,et al. The Sloan Digital Sky Survey Quasar Survey: Quasar Luminosity Function from Data Release 3 , 2006, astro-ph/0601434.
[29] P. Martini,et al. Coevolution of Black Holes and Galaxies , 2004 .
[30] G. Zamorani,et al. Most Supermassive Black Holes Must Be Rapidly Rotating , 2001, astro-ph/0112413.
[31] Andrew King,et al. Growing supermassive black holes by chaotic accretion , 2006 .
[32] Ž. Ivezić,et al. The Radio-Loud Fraction of Quasars is a Strong Function of Redshift and Optical Luminosity , 2006, astro-ph/0611453.
[33] A. Mazure,et al. The VIMOS-VLT deep survey - Evolution of the galaxy luminosity function up to z = 2 in first epoch data , 2004, astro-ph/0409134.
[34] A. Marconi,et al. The Relation between Black Hole Mass, Bulge Mass, and Near-Infrared Luminosity , 2003, astro-ph/0304274.
[35] F. Schweizer. Observational Evidence for Interactions and Mergers , 1996 .
[36] The Mass Function of Active Black Holes in the Local Universe , 2007 .
[37] G. Kauffmann,et al. The many lives of active galactic nuclei: cooling flows, black holes and the luminosities and colour , 2005, astro-ph/0508046.
[38] A. Merloni,et al. A synthesis model for AGN evolution: supermassive black holes growth and feedback modes , 2008, 0805.2499.
[39] D. Kirkman,et al. The transverse proximity effect in the z∼ 2 Lyman α forest suggests quasi-stellar object episodic lifetimes of ∼1 Myr , 2008, 0809.2277.
[40] G. Richards,et al. An Observational Determination of the Bolometric Quasar Luminosity Function , 2006, astro-ph/0605678.
[41] A. Marconi,et al. Local supermassive black holes, relics of active galactic nuclei and the X-ray background , 2003, astro-ph/0311619.
[42] Oxford,et al. The COMBO-17 survey: Evolution of the galaxy luminosity function from 25,000 galaxies with 0.2 < z < 1.2 , 2002, astro-ph/0208345.