scholarly journals Eccentricity without Measuring Eccentricity: Discriminating among Stellar Mass Black Hole Binary Formation Channels

2021 ◽  
Vol 914 (2) ◽  
pp. 75
Author(s):  
Lisa Randall ◽  
Zhong-Zhi Xianyu
2007 ◽  
Vol 665 (1) ◽  
pp. L51-L54 ◽  
Author(s):  
J. Albert ◽  
E. Aliu ◽  
H. Anderhub ◽  
P. Antoranz ◽  
A. Armada ◽  
...  

2003 ◽  
Vol 405 (2) ◽  
pp. 505-511 ◽  
Author(s):  
R. Barnard ◽  
J. P. Osborne ◽  
U. Kolb ◽  
K. N. Borozdin

2016 ◽  
Vol 832 (1) ◽  
pp. L2 ◽  
Author(s):  
Carl L. Rodriguez ◽  
Michael Zevin ◽  
Chris Pankow ◽  
Vasilliki Kalogera ◽  
Frederic A. Rasio

1998 ◽  
Vol 58 (6) ◽  
Author(s):  
Kunihito Ioka ◽  
Takeshi Chiba ◽  
Takahiro Tanaka ◽  
Takashi Nakamura

2006 ◽  
Vol 469 (3) ◽  
pp. 873-873 ◽  
Author(s):  
R. Barnard ◽  
U. C. Kolb ◽  
J. P. Osborne

2013 ◽  
Vol 87 (10) ◽  
Author(s):  
Davide Gerosa ◽  
Michael Kesden ◽  
Emanuele Berti ◽  
Richard O’Shaughnessy ◽  
Ulrich Sperhake

2019 ◽  
Vol 15 (S359) ◽  
pp. 37-39
Author(s):  
Benjamin L. Davis ◽  
Nandini Sahu ◽  
Alister W. Graham

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.


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