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Cited by 408

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Ejection of Hypervelocity Stars by the (Binary) Black Hole in the Galactic Center

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Yu, Qingjuan, Tremaine, Scott·2003·The Astrophysical Journal

Abstract

We study three processes that eject hypervelocity (>10 3 km s -1 ) stars from the Galactic center: (1) close encounters of two single stars, (2) tidal breakup of binary stars by the central black hole, as originally proposed by Hills, and (3) three-body interactions between a star and a binary black hole (BBH). Mechanism 1 expels hypervelocity stars to the solar radius, R 0 = 8 kpc, at a negligible rate, ~10 -11 yr -1 . Mechanism 2 expels hypervelocity stars at a rate ~10 -5 (η/0.1) yr -1 , where η is the fraction of stars in binaries with semimajor axis a b ≲ 0.3 AU. For solar mass stars, the corresponding number of hypervelocity stars within the solar radius is ~60(η/0.1)( a b /0.1 AU) 1/2 . For mechanism 3, Sgr A* is assumed to be one component of a BBH. We constrain the allowed parameter space (semimajor axis, mass ratio) of the BBH. In the allowed region (for example, a semimajor axis of 0.5 × 10 -3 pc and a mass ratio of 0.01), the rate of ejection of hypervelocity stars can be as large as ~10 -4 yr -1 , and the expected number of hypervelocity stars within the solar radius can be as large as ~10 3 . Hypervelocity stars may be detectable by the next generation of large-scale optical surveys.

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Metadata

Authors
Yu, Q., & Tremaine, S.
Venue
The Astrophysical Journal
Published
2003-12-20
Volume
599
Issue
2
Pages
1129-1138
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W2153555990
Cited by
408
References
33
FWCI
9.47
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: Ejection of Hypervelocity Stars by the (Binary) Black Hole in the Galactic Center. https://app.cochat.ai/papers/10.1086/379546
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Yu, Q., & Tremaine, S. (2003). Ejection of Hypervelocity Stars by the (Binary) Black Hole in the Galactic Center. The Astrophysical Journal. https://doi.org/10.1086/379546

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