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The black hole spin in coalescing binary black holes and high-mass X-ray binaries

Published online by Cambridge University Press:  30 December 2019

Y. Qin ,
T. Fragos ,
G. Meynet ,
P. Marchant ,
V. Kalogera ,
J. Andrews ,
M. Sørensen  and
H. F. Song
Y. Qin
Affiliation:
Geneva Observatory, University of Geneva, CH-1290 Sauverny, Switzerland email: [email protected] Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA) and Department of Physics and Astrophysics, Northwestern University, Evanston, IL 60208
T. Fragos
Affiliation:
Geneva Observatory, University of Geneva, CH-1290 Sauverny, Switzerland email: [email protected]
G. Meynet
Affiliation:
Geneva Observatory, University of Geneva, CH-1290 Sauverny, Switzerland email: [email protected]
P. Marchant
Affiliation:
Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA) and Department of Physics and Astrophysics, Northwestern University, Evanston, IL 60208
V. Kalogera
Affiliation:
Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA) and Department of Physics and Astrophysics, Northwestern University, Evanston, IL 60208
J. Andrews
Affiliation:
Foundation for Research and Technology - Hellas, IESL, Voutes, 71110 Heraklion, Greece Physics Department & Institute of Theoretical & Computational Physics, University of Crete, 71003 Heraklion, Crete, Greece
M. Sørensen
Affiliation:
Geneva Observatory, University of Geneva, CH-1290 Sauverny, Switzerland email: [email protected]
H. F. Song
Affiliation:
College of Physics, Guizhou University, Guiyang City, Guizhou Province, 550025, P.R. China Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650011
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Abstract

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The six LIGO detections of merging black holes (BHs) allowed to infer slow spin values for the two pre-merging BHs. The three cases where the spins of the BHs can be determined in high-mass X-ray binaries (HMXBs) show that those BHs have high spin values. We discuss here scenarios explaining these differences in spin properties in these two classes of object.

Keywords

binaries: close binary starsX-rays: binariesblack holegravitational waves
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium S346: High-mass X-ray Binaries: Illuminating the Passage from Massive Binaries to Merging Compact Objects , August 2018 , pp. 426 - 432
Copyright
© International Astronomical Union 2019 

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