Constraining a black hole companion for M87* through imaging by the Event Horizon Telescope
Abstract
The Event Horizon Telescope, a global very long baseline interferometric array observing at a wavelength of 1.3 mm, detected the first image of the M87 supermassive black hole (SMBH). M87 is a giant elliptical galaxy at the centre of the Virgo cluster, which is expected to have formed through merging of cluster galaxies. Consequently M87* hosted mergers of black holes through dynamical friction and could have one or multiple binary companions with a low mass ratio at large separations. We show that a long-term monitoring of the M87 SMBH image over ∼1 yr with absolute positional accuracy of 1 ≈ μas could detect such binary companions and exclude a large parameter space in semimajor axis (a0) and mass ratio (q), which is currently not constrained. Moreover, the presence of the accretion disc around M87* excludes a binary companion with a0 ≈ of the order of a milliparsec, as otherwise the accretion disc would have been tidally disrupted.
- Publication:
-
Monthly Notices of the Royal Astronomical Society
- Pub Date:
- September 2019
- DOI:
- 10.1093/mnrasl/slz108
- arXiv:
- arXiv:1905.06835
- Bibcode:
- 2019MNRAS.488L..90S
- Keywords:
-
- radio continuum: general;
- Galaxies: Supermassive black holes;
- Astrophysics - Astrophysics of Galaxies;
- Astrophysics - High Energy Astrophysical Phenomena;
- High Energy Physics - Theory
- E-Print:
- accepted for publication at MNRAS Letters