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2020ApJ...902..103I - Astrophys. J., 902, 103-103 (2020/October-3)
Radiation magnetohydrodynamic simulations of sub-Eddington accretion flows in AGNs: origin of soft X-ray excess and rapid time variabilities.
IGARASHI T., KATO Y., TAKAHASHI H.R., OHSUGA K., MATSUMOTO Y. and MATSUMOTO R.
Abstract (from CDS):
Abstract Copyright: © 2020. The American Astronomical Society. All rights reserved.
Journal keyword(s): Galaxy accretion disks - Active galactic nuclei - Radiative magnetohydrodynamics
Simbad objects: 7
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