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2017MNRAS.466.2236D - Mon. Not. R. Astron. Soc., 466, 2236-2241 (2017/April-1)
Modelling the light curves of ultraluminous X-ray sources as precession.
DAUSER T., MIDDLETON M. and WILMS J.
Abstract (from CDS):
Abstract Copyright: © 2016 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society
Journal keyword(s): accretion, accretion discs - black hole physics - pulsars: individual: NGC 5907 ULX-1 - X-rays: binaries - X-rays: binaries
Simbad objects: 7
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