Spins of the Supermassive Black Hole in M87: New Constraints from TeV Observations
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[1] Chen Hu,et al. Early Growth of Massive Black Holes in Quasars , 2007, 0712.0523.
[2] A. Babul,et al. Models for jet power in elliptical galaxies: a case for rapidly spinning black holes , 2006, astro-ph/0612354.
[3] A. R. Bazer-Bachi,et al. Fast Variability of TeraElectron Volt γ Rays from the Radio Galaxy M87 , 2006, Science.
[4] L. Brenneman,et al. Constraining Black Hole Spin via X-Ray Spectroscopy , 2006, astro-ph/0608502.
[5] L. Ho,et al. Evidence for Rapidly Spinning Black Holes in Quasars , 2006, astro-ph/0603813.
[6] M. Rees,et al. ApJ, in press Preprint typeset using L ATEX style emulateapj v. 04/03/99 THE DISTRIBUTION AND COSMIC EVOLUTION OF MASSIVE BLACK HOLE SPINS , 2004 .
[7] R. Maiolino,et al. Local supermassive black holes, relics of active galactic nuclei and the X-ray background , 2003, astro-ph/0311619.
[8] Tiziana Di Matteo,et al. Accretion onto the Supermassive Black Hole in M87 , 2002, astro-ph/0202238.
[9] J. C. Lee,et al. A long hard look at MCG–6-30-15 with XMM-Newton , 2002, astro-ph/0311473.
[10] S. Tremaine,et al. Observational constraints on growth of massive black holes , 2002, astro-ph/0203082.
[11] William B. Sparks,et al. Deep 10 Micron Imaging of M87 , 2001 .
[12] S. Molendi,et al. XMM-EPIC observation of MCG-6-30-15: direct evidence for the extraction of energy from a spinning black hole? , 2001, astro-ph/0110520.
[13] F. Yuan,et al. The Role of the Outer Boundary Condition in Accretion Disk Models: Theory and Application , 2000, astro-ph/0002068.
[14] John A. Biretta,et al. Formation of the radio jet in M87 at 100 Schwarzschild radii from the central black hole , 1999, Nature.
[15] Cambridge,et al. Low‐radiative‐efficiency accretion in the nuclei of elliptical galaxies , 1999, astro-ph/9905053.
[16] S. Mineshige,et al. Spectrum of Optically Thin Advection-dominated Accretion Flow around a Black Hole: Application to Sagittarius A* , 1997, astro-ph/9708234.
[17] W. Sparks,et al. The Supermassive Black Hole of M87 and the Kinematics of Its Associated Gaseous Disk , 1997, astro-ph/9706252.
[18] R. Narayan,et al. Global Structure and Dynamics of Advection-dominated Accretion Flows around Black Holes , 1996, astro-ph/9607019.
[19] Cambridge,et al. The 'Quiescent' black hole in M87 , 1996, astro-ph/9610097.
[20] Geoffrey V. Bicknell,et al. Understanding the Kiloparsec-Scale Structure of M87 , 1996 .
[21] R. Narayan,et al. Advection dominated accretion: Underfed black holes and neutron stars , 1994, astro-ph/9411059.
[22] H. Ford,et al. HST FOS spectroscopy of M87: Evidence for a disk of ionized gas around a massive black hole , 1994 .
[23] R. Narayan,et al. Advection-dominated Accretion: A Self-similar Solution , 1994, astro-ph/9403052.
[24] E. Turner,et al. Remnants of the quasars. , 1992 .
[25] A compact radio source in the nucleus of M87 , 1986, Nature.
[26] D. Graham,et al. 6-cm VLBI observations of compact radio sources , 1981 .
[27] K. Thorne. Disk-Accretion onto a Black Hole. II. Evolution of the Hole , 1974 .
[28] J. Bardeen,et al. Kerr Metric Black Holes , 1970, Nature.
[29] R. Gould,et al. Pair production in photon-photon collisions. , 1967 .