SUPERMASSIVE BLACK HOLE AT THE GALACTIC CENTER
We derive an analytical expression of a shadow size as a function of a charge in the Reissner - Nordstr?m (RN) metric. Using the derived expression we consider shadows for negative tidal charges and charges corresponding to naked singularities q=Q2/M2>1, where Q and M are black hole charge and mass, respectively.
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THE MURMUR OF THE HIDDEN MONSTER: CHANDRA 'S DECADAL VIEW OF THE SUPERMASSIVE BLACK HOLE IN M31 [PDF]
Jun Yi Koay +7 more
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INTERRUPTION OF TIDAL-DISRUPTION FLARES BY SUPERMASSIVE BLACK HOLE BINARIES [PDF]
F.K. Liu +5 more
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X-ray flares from the stellar tidal disruption by a candidate supermassive black hole binary. [PDF]
Shu X +10 more
europepmc +1 more source
The Growth of the Earliest Supermassive Black Holes and Their Contribution to Reionization [PDF]
Zoltán Haiman +2 more
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Eötvös Experiments with Supermassive Black Holes [PDF]
Asha Asvathaman, Jeremy Heyl, Lam Hui
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The effects of super-Eddington accretion and feedback on the growth of early supermassive black holes and galaxies [PDF]
Filip Huško +5 more
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The missing x-rays in Sgr A*: evidence for - not against - a\n supermassive black hole [PDF]
H. Falcke, Peter L. Biermann
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Supermassive black holes : the local supermassive black hole mass function
Over recent years there has been an increase of the number of secure supermassive black hole (SMBH) detections. These SMBH measurements have lead astronomers to establish well defined empirical relationships between the SMBH mass and some of the properties of the host galaxy.
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Supermassive black holes as giant Bose-Einstein condensates [PDF]
Theo M. Nieuwenhuizen
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