scholarly journals What Does the Local Black Hole Mass Distribution Tell Us About the Evolution of the Quasar Luminosity Function?

2006 ◽  
pp. 106-108 ◽  
Author(s):  
Luca Ciotti ◽  
Zoltan Haiman ◽  
Jeremiah P. Ostriker
Keyword(s):  
Black Hole ◽  
Mass Distribution ◽  
Luminosity Function ◽  
Black Hole Mass

scholarly journals The Impact of Pair-instability Mass Loss on the Binary Black Hole Mass Distribution

2019 ◽  
Vol 882 (2) ◽  
pp. 121 ◽  
Author(s):  
Simon Stevenson ◽  
Matthew Sampson ◽  
Jade Powell ◽  
Alejandro Vigna-Gómez ◽  
Coenraad J. Neijssel ◽  
...  
Keyword(s):  
Black Hole ◽  
Mass Loss ◽  
Mass Distribution ◽  
Black Hole Mass ◽  
Binary Black Hole ◽  
The Impact

scholarly journals THE BLACK HOLE MASS DISTRIBUTION IN THE GALAXY

2010 ◽  
Vol 725 (2) ◽  
pp. 1918-1927 ◽  
Author(s):  
Feryal Özel ◽  
Dimitrios Psaltis ◽  
Ramesh Narayan ◽  
Jeffrey E. McClintock
Keyword(s):  
Black Hole ◽  
Mass Distribution ◽  
Black Hole Mass ◽  
The Galaxy

Stability of the parameters of the Stellar black-hole mass distribution estimated using nonparametric methods

2014 ◽  
Vol 58 (3) ◽  
pp. 113-125 ◽  
Author(s):  
V. S. Petrov ◽  
A. M. Cherepashchuk ◽  
E. A. Antokhina
Keyword(s):  
Black Hole ◽  
Mass Distribution ◽  
Nonparametric Methods ◽  
Black Hole Mass

scholarly journals Tidal Disruption Events and stellar-mass black holes in OGLE and Gaia surveys

2016 ◽  
Vol 12 (S324) ◽  
pp. 127-131
Author(s):  
Łukasz Wyrzykowski ◽  
A. Hamanowicz ◽  
K. A. Rybicki
Keyword(s):  
Black Holes ◽  
Black Hole ◽  
Mass Distribution ◽  
Milky Way ◽  
Black Hole Mass ◽  
Tidal Disruption ◽  
Massive Black Holes ◽  
Mass Growth ◽  
Highly Active ◽  
Different Levels

AbstractTidal Disruption Events (TDE) allow to probe the super massive black holes (SMBH) in the cores of galaxies and could be a source of black hole mass growth. We present the search for candidates for TDEs conducted within OGLE and Gaia surveys. Our preliminary results indicate that TDEs can occur in cores of galaxies exhibiting different levels of activity, from quiescent, through weak-AGNs to highly active QSOs. We also present how Gaia can help study the mass distribution of Milky Way single black holes via microlensing.

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