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
Publication year
2013Source
Monthly Notices of the Royal Astronomical Society, 433, 2, (2013), pp. 1023-1038ISSN
Publication type
Article / Letter to editor
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Organization
Astrophysics
Journal title
Monthly Notices of the Royal Astronomical Society
Volume
vol. 433
Issue
iss. 2
Page start
p. 1023
Page end
p. 1038
Subject
AstronomyThis item appears in the following Collection(s)
- Academic publications [245396]
- Electronic publications [132943]
- Faculty of Science [37565]
- Open Access publications [106466]
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