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2018
AbstractThe supermassive BH at the center of our Galaxy. Formation and evolution of SMBH binaries. Perspective for detection with LISA. Extreme mass ratio inspirals (EMRIs). Computation of the EMRI’s waveform with the self-force approach. Stochastic backgrounds of gravitational waves produced by SMBH binaries. Perspective for detection at pulsar timing
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AbstractThe supermassive BH at the center of our Galaxy. Formation and evolution of SMBH binaries. Perspective for detection with LISA. Extreme mass ratio inspirals (EMRIs). Computation of the EMRI’s waveform with the self-force approach. Stochastic backgrounds of gravitational waves produced by SMBH binaries. Perspective for detection at pulsar timing
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Supermassive Black Holes in Quasars
AIP Conference Proceedings, 2006Computing the basic accretion parameters for the supermassive black holes expected to be present in quasars is still a major challenge. In this paper we stress how a systematization of observational properties through the so‐called “eigenvector 1” of quasars helps to develop a clearer view of the structure and dynamics of the Broad Line Region ...
Jack W. Sulentic +2 more
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Supermassive black hole in M87 [PDF]
Physics World, 1994 For two decades, astronomers have hunted for definitive proof of the existence of supermassive black holes in the centres of galaxies. Now, observations with the Hubble Space Telescope (HST), led by Holland Ford of Johns Hopkins University, have prosecuted the case of the galaxy M87 in a manner that would at least satisfy the civil if not criminal ...
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Tidal Disruption of Stars by Supermassive Black Holes
, 2015Nicholas C. Stone
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