A long-term X-ray monitoring of the ultraluminous X-ray source NGC5408X-1 with Swift reveals the presence of dips but no orbital period

Author： Gris F.

Publisher： Oxford University Press

ISSN： 0035-8711

Source： Monthly Notices of the Royal Astronomical Society, Vol.433, Iss.2, 2013-01, pp. : 1023-1038

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