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2021ApJ...906...34K - Astrophys. J., 906, 34-34 (2021/January-1)
Generally applicable formalism for modeling the observable signatures of inflows, outflows, and moving coronal plasma close to Kerr black holes.
KRAWCZYNSKI H.
Abstract (from CDS):
Abstract Copyright: © 2021. The American Astronomical Society. All rights reserved.
Journal keyword(s): Quasars - Black hole physics - Kerr black holes
Simbad objects: 3
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