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Volumn 365, Issue 3, 2001, Pages 508-513
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The detection of a 1.4-h period in RW Ursa Minoris - candidate for shortest recorded orbital period nova
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Author keywords
Accretion; Accretion discs; Binaries: close; Cataclysmic variables; Individual: RW Umi; Novae; White dwarfs
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Indexed keywords
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EID: 0034800366
PISSN: 00046361
EISSN: None
Source Type: Journal
DOI: 10.1051/0004-6361:20000150 Document Type: Article |
Times cited : (9)
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References (40)
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