SIMBAD references

2019MNRAS.486.3118D - Mon. Not. R. Astron. Soc., 486, 3118-3123 (2019/July-1)

Modelling general-relativistic disc in OJ 287.

DYBA W., MACH P. and MALEC E.

Abstract (from CDS):

We model a self-gravitating disc in Keplerian motion around the primary black hole in the binary black hole system OJ 287, employing a consistently general-relativistic approach. Our models satisfy either geometric requirements on the disc or the requirements on its mass density found by Lehto, Valtonen, and their coworkers. It is plausible that essential observational features of OJ 287 can be obtained via the general-relativistic description of the Bondi-Hoyle-Lyttleton transits through the disc, within the framework of radiation hydrodynamics.

Abstract Copyright: © 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): black hole physics - gravitation - hydrodynamics - quasars: individual: (OJ 287)

Simbad objects: 1

goto Full paper

goto View the references in ADS

To bookmark this query, right click on this link: simbad:2019MNRAS.486.3118D and select 'bookmark this link' or equivalent in the popup menu