scholarly journals Revisit the Fundamental Plane of black hole activity from sub-Eddington to quiescent state

2015 ◽  
Vol 453 (4) ◽  
pp. 3448-3455 ◽  
Author(s):  
Ai-Jun Dong ◽  
Qingwen Wu



2020 ◽  
Vol 498 (4) ◽  
pp. 5511-5511
Author(s):  
Caner Ünal ◽  
Abraham Loeb


2014 ◽  
Vol 788 (2) ◽  
pp. L22 ◽  
Author(s):  
Kayhan Gültekin ◽  
Edward M. Cackett ◽  
Ashley L. King ◽  
Jon M. Miller ◽  
Jason Pinkney


New Astronomy ◽  
2006 ◽  
Vol 11 (8) ◽  
pp. 567-576 ◽  
Author(s):  
A. Merloni ◽  
E. Körding ◽  
S. Heinz ◽  
S. Markoff ◽  
T. DiMatteo ◽  
...  
Keyword(s):  


2003 ◽  
Vol 595 (2) ◽  
pp. 624-630 ◽  
Author(s):  
R. Falomo ◽  
J. K. Kotilainen ◽  
N. Carangelo ◽  
A. Treves


2006 ◽  
Vol 645 (2) ◽  
pp. 890-899 ◽  
Author(s):  
Ran Wang ◽  
Xue‐Bing Wu ◽  
Min‐Zhi Kong


2015 ◽  
Vol 450 (3) ◽  
pp. 2317-2326 ◽  
Author(s):  
Payaswini Saikia ◽  
Elmar Körding ◽  
Heino Falcke
Keyword(s):  


2018 ◽  
Vol 477 (2) ◽  
pp. 2119-2127 ◽  
Author(s):  
Payaswini Saikia ◽  
Elmar Körding ◽  
Salome Dibi
Keyword(s):  


2007 ◽  
Vol 3 (S245) ◽  
pp. 219-222
Author(s):  
Philip F. Hopkins

AbstractWe study observed correlations between supermassive black hole (BHs) and the properties of their host galaxies, and show that the observations define a BH “fundamental plane” (BHFP), of the form $\mbh\propto\sigma^{3.0\pm0.3}\,\re^{0.43\pm0.19}$ or $\mbh\propto\mstar^{0.54\pm0.17}\,\sigma^{2.2\pm0.5}$, analogous to the FP of elliptical galaxies. The BHFP is preferred over a simple relation between MBH and any of σ, M*, Mdyn, or Re alone at > 3 σ (99.9%) significance. The existence of this BHFP has important implications for the formation of supermassive BHs and the masses of the very largest black holes, and immediately resolves several apparent conflicts between the BH masses expected and measured for outliers in both the MBH − σ and MBH − M* relations.



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