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Cited by 359

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THE MASS OF THE BLACK HOLE IN CYGNUS X-1

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Orosz, Jerome A., McClintock, Jeffrey E., Aufdenberg, Jason P., Remillard, Ronald A., Reid, Mark J., Narayan, Ramesh, Gou, Lijun·2011·The Astrophysical Journal

Abstract

Cygnus X-1 is a binary star system that is comprised of a black hole and a massive giant companion star in a tight orbit. Building on our accurate distance measurement reported in the preceding paper, we first determine the radius of the companion star, thereby constraining the scale of the binary system. To obtain a full dynamical model of the binary, we use an extensive collection of optical photometric and spectroscopic data taken from the literature. By using all of the available observational constraints, we show that the orbit is slightly eccentric (both the radial velocity and photometric data independently confirm this result) and that the companion star rotates roughly 1.4 times its pseudosynchronous value. We find a black hole mass of M = 14.8 ± 1.0 M ☉ , a companion mass of M opt = 19.2 ± 1.9 M ☉ , and the angle of inclination of the orbital plane to our line of sight of i = 27.1 ± 0.8 deg.

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Metadata

Authors
Orosz, J. A., McClintock, J. E., Aufdenberg, J. P., Remillard, R. A., Reid, M. J., Narayan, R., & Gou, L.
Venue
The Astrophysical Journal
Published
2011-11-09
Volume
742
Issue
2
Pages
84
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W2096503596
Cited by
359
References
1
FWCI
12.10
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: THE MASS OF THE BLACK HOLE IN CYGNUS X-1. https://app.cochat.ai/papers/10.1088/0004-637x/742/2/84
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Orosz, J. A., McClintock, J. E., Aufdenberg, J. P., Remillard, R. A., Reid, M. J., Narayan, R., & Gou, L. (2011). THE MASS OF THE BLACK HOLE IN CYGNUS X-1. The Astrophysical Journal. https://doi.org/10.1088/0004-637x/742/2/84

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