scholarly journals RX J0042.3+4115: A stellar mass black hole binary identified in M 31

2003 ◽  
Vol 405 (2) ◽  
pp. 505-511 ◽  
Author(s):  
R. Barnard ◽  
J. P. Osborne ◽  
U. Kolb ◽  
K. N. Borozdin
Keyword(s):  
Black Hole ◽  
Stellar Mass ◽  
Black Hole Binary ◽  
M 31

scholarly journals RX J0042.3+4115: a stellar mass black hole binary identified in M 31, and other papers

2006 ◽  
Vol 469 (3) ◽  
pp. 873-873 ◽  
Author(s):  
R. Barnard ◽  
U. C. Kolb ◽  
J. P. Osborne
Keyword(s):  
Black Hole ◽  
Stellar Mass ◽  
Black Hole Binary ◽  
M 31

scholarly journals Very High Energy Gamma-Ray Radiation from the Stellar Mass Black Hole Binary Cygnus X-1

2007 ◽  
Vol 665 (1) ◽  
pp. L51-L54 ◽  
Author(s):  
J. Albert ◽  
E. Aliu ◽  
H. Anderhub ◽  
P. Antoranz ◽  
A. Armada ◽  
...  
Keyword(s):  
Black Hole ◽  
Gamma Ray ◽  
High Energy ◽  
Stellar Mass ◽  
High Energy Gamma ◽  
Very High Energy ◽  
Energy Gamma ◽  
Black Hole Binary ◽  
Very High

Substructure in black hole scaling diagrams and implications for the coevolution of black holes and galaxies

2019 ◽  
Vol 15 (S359) ◽  
pp. 37-39
Author(s):  
Benjamin L. Davis ◽  
Nandini Sahu ◽  
Alister W. Graham
Keyword(s):  
Black Hole ◽  
Stellar Mass ◽  
Host Galaxy ◽  
Scaling Relations ◽  
Black Hole Mass ◽  
Physical Processes ◽  
Stellar Velocity ◽  
Galaxy Sample ◽  
Evolutionary Paths ◽  
Black Hole Masses

AbstractOur multi-component photometric decomposition of the largest galaxy sample to date with dynamically-measured black hole masses nearly doubles the number of such galaxies. We have discovered substantially modified scaling relations between the black hole mass and the host galaxy properties, including the spheroid (bulge) stellar mass, the total galaxy stellar mass, and the central stellar velocity dispersion. These refinements partly arose because we were able to explore the scaling relations for various sub-populations of galaxies built by different physical processes, as traced by the presence of a disk, early-type versus late-type galaxies, or a Sérsic versus core-Sérsic spheroid light profile. The new relations appear fundamentally linked with the evolutionary paths followed by galaxies, and they have ramifications for simulations and formation theories involving both quenching and accretion.

Parameters of V404 Cyg—A black-hole binary

2004 ◽  
Vol 48 (12) ◽  
pp. 1019-1028 ◽  
Author(s):  
A. M. Cherepashchuk ◽  
N. V. Borisov ◽  
M. K. Abubekerov ◽  
D. K. Klochkov ◽  
É. A. Antokhina
Keyword(s):  
Black Hole ◽  
Black Hole Binary

scholarly journals A reduced orbital period for the supermassive black hole binary candidate in the quasar PG 1302-102?

2015 ◽  
Vol 452 (3) ◽  
pp. 2540-2545 ◽  
Author(s):  
D. J. D'Orazio ◽  
Z. Haiman ◽  
P. Duffell ◽  
B. D. Farris ◽  
A. I. MacFadyen
Keyword(s):  
Black Hole ◽  
Orbital Period ◽  
Supermassive Black Hole ◽  
Black Hole Binary

scholarly journals Black hole binary OJ287 as a testing platform for general relativity

2014 ◽  
Vol 484 ◽  
pp. 012025
Author(s):  
M J Valtonen ◽  
A Gopakumar ◽  
S Mikkola ◽  
K Wiik ◽  
H J Lehto
Keyword(s):  
General Relativity ◽  
Black Hole ◽  
Testing Platform ◽  
Black Hole Binary
Sign in / Sign up

Export Citation Format

Share Document