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2013MNRAS.433.1023G - Mon. Not. R. Astron. Soc., 433, 1023-1038 (2013/August-1)
A long-term X-ray monitoring of the ultraluminous X-ray source NGC 5408 X-1 with Swift reveals the presence of dips but no orbital period.
GRISE F., KAARET P., CORBEL S., CSEH D. and FENG H.
Abstract (from CDS):
Abstract Copyright: © 2013 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society (2013)
Journal keyword(s): accretion, accretion discs - X-rays: binaries - X-rays: individual: NGC 5408 X-1
Simbad objects: 18
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