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2022MNRAS.514..234Y - Mon. Not. R. Astron. Soc., 514, 234-248 (2022/July-3)
The origin of UV/optical emission in the black hole low-mass X-ray binary Swift J1753.5-0127.
YANG P., ZHANG G., RUSSELL D.M., GELFAND J.D., MENDEZ M., WANG J. and LYU M.
Abstract (from CDS):
Abstract Copyright: © 2022 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society
Journal keyword(s): accretion, accretion discs - stars: black holes - X-rays: binaries - X-rays: individual: Swift J1753.5-0127
Simbad objects: 7
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