SIMBAD references

2021ApJ...916..108Z - Astrophys. J., 916, 108-108 (2021/August-1)

Estimating the black hole spin for the X-ray binary MAXI J1820+070.

ZHAO X., GOU L., DONG Y., TUO Y., LIAO Z., LI Y., JIA N., FENG Y. and STEINER J.F.

Abstract (from CDS):

MAXI J1820+070 is a newly discovered black hole X-ray binary, whose dynamical parameters, namely the black hole mass, the inclination angle, and the source distance, have recently been estimated. Insight-HXMT have observed its entire outburst from 2018 March 14. In this work, we attempted to estimate the spin parameter a*, using the continuum-fitting method and applying a fully relativistic thin disk model to the soft-state spectra obtained by Insight-HXMT. It is well known that a* is strongly dependent on three dynamical parameters in this method, and we have examined two sets of parameters. Adopting our preferred parameters: M = 8.48–0.72+0.79M☉, i = 63° ± 3°, and D = 2.96 ± 0.33 kpc, we found a slowly spinning black hole of a* = 0.14 ± 0.09 (1σ), which gives a prograde spin parameter as the majority of other systems show. It is also possible for the black hole to have a retrograde spin (less than 0) if different dynamical parameters are taken.

Abstract Copyright: © 2021. The American Astronomical Society. All rights reserved.

Journal keyword(s): Black hole physics - X-ray binary stars

Simbad objects: 1

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