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2019ApJ...887..184T - Astrophys. J., 887, 184-184 (2019/December-3)
The spin of the black hole GRS 1716-249 determined from the hard intermediate state.
TAO L., TOMSICK J.A., QU J., ZHANG S., ZHANG S. and BU Q.
Abstract (from CDS):
Abstract Copyright: © 2019. The American Astronomical Society. All rights reserved.
Journal keyword(s): Accretion - X-ray binary stars - Rotating black holes - Black Hole physics
Simbad objects: 4
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