C.D.S. - SIMBAD4 rel 1.7 - 2019.10.14CEST21:31:05

2019MNRAS.482.3206W - Mon. Not. R. Astron. Soc., 482, 3206-3218 (2019/January-3)

Hypervelocity binaries from close encounters with a SMBH-IMBH binary: orbital properties and diagnostics.


Abstract (from CDS):

Hypervelocity binaries (HVBs) can be produced by a close encounter between stellar binaries and supermassive black hole (SMBH)-intermediate massive black hole (IMBH) binaries. We perform scattering experiments between tight stellar binaries and an SMBH-IMBH binary (within the observationally allowed parameters), using high-precision N-body integrations. Simulation results show that only a few HVBs can be produced in the Galactic centre if it harbours a 4 x 103 M IMBH. However, we find that tight HVBs can be efficiently produced in prograde coplanar orbits with respect to the SMBH-IMBH binary. Therefore, the trajectories of the HVBs provide a promising way to constrain the IMBH orbital plane, if one exists. More importantly, we find that the ejected tight binaries are eccentric. For other galaxies hosting equal-mass SMBH binaries for which the HVB ejection rate is much higher relative to SMBH-IMBH binaries, these ejected compact binaries constitute promising extragalactic merger sources that could be detected by gravitational wave detectors.

Abstract Copyright: © 2018 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): black hole physics

Simbad objects: 5

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Number of rows : 5

N Identifier Otype ICRS (J2000)
ICRS (J2000)
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2019
1 HE 0437-5439 HS* 04 38 12.7828185490 -54 33 11.840105637 15.37 16.18 16.42     sdB+F 59 0
2 NAME LMC G 05 23 34.6 -69 45 22     0.4     ~ 14317 1
3 PB 3877 WD* 12 11 50.2653712012 +14 37 16.205983104   17.5       DAB 17 0
4 NAME Sgr A* X 17 45 40.03599 -29 00 28.1699           ~ 3262 3
5 NAME Gal Center reg 17 45 40.04 -29 00 28.1           ~ 10995 0

    Equat.    Gal    SGal    Ecl

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