Gravitational interactions of stars with supermassive black hole binaries – II. Hypervelocity stars

Journal Article · 14 October 2018 · Monthly Notices of the Royal Astronomical Society

DOI: https://doi.org/10.1093/mnras/sty2786 · OSTI ID:1481794

Darbha, Siva ^[1]; Coughlin, Eric R.  ^[2]; Kasen, Daniel ^[3]; Quataert, Eliot ^[4]

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1. Department of Physics, University of California, Berkeley, Berkeley, CA 94720, USA
2. Department of Astronomy and Theoretical Astrophysics Center, University of California, Berkeley, Berkeley, CA 94720, USA, Columbia Astrophysics Laboratory, Columbia University, New York, NY 10027, USA
3. Department of Physics, University of California, Berkeley, Berkeley, CA 94720, USA, Department of Astronomy and Theoretical Astrophysics Center, University of California, Berkeley, Berkeley, CA 94720, USA, Nuclear Science Division, Lawrence Berkeley National Laboratory, Berkeley, CA 94720, USA
4. Department of Physics, University of California, Berkeley, Berkeley, CA 94720, USA, Department of Astronomy and Theoretical Astrophysics Center, University of California, Berkeley, Berkeley, CA 94720, USA

Not Available

• Research Organization: Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States). National Energy Research Scientific Computing Center (NERSC); Univ. of California, Oakland, CA (United States)
• Sponsoring Organization: USDOE; USDOE Office of Science (SC)
• Grant/Contract Number: AC02-05CH11231
• OSTI ID: 1481794
• Journal Information: Monthly Notices of the Royal Astronomical Society, Journal Name: Monthly Notices of the Royal Astronomical Society Journal Issue: 2 Vol. 482; ISSN 0035-8711
• Publisher: Oxford University PressCopyright Statement
• Country of Publication: United Kingdom
• Language: English