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2008MNRAS.389..423P - Mon. Not. R. Astron. Soc., 389, 423-428 (2008/September-1)
Origin of X-ray emission from transient black hole candidates in quiescence.
PSZOTA G., ZHANG H., YUAN F. and CUI W.
Abstract (from CDS):
Abstract Copyright: © 2008 The Authors. Journal compilation © 2008 RAS
Journal keyword(s): radiation mechanisms: non-thermal - radiation mechanisms: thermal - stars: individual: XTE J1550-564 - stars: individual: GRO J1655-40 - stars: individual: V404 Cyg - X-rays: binaries
Simbad objects: 5
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