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2000PASP..112.1584P - Publ. Astron. Soc. Pac., 112, 1584-1594 (2000/December-0)
Superhumps in cataclysmic binaries. XIX. DV Ursae majoris.
PATTERSON J., VANMUNSTER T., SKILLMAN D.R., JENSEN L., STULL J., MARTIN B., COOK L.M., KEMP J. and KNIGGE C.
Abstract (from CDS):
We also report photometry at quiescence, which separates the luminous contributions of the white dwarf, accretion disk, and secondary star. We estimate a distance of 350±120 pc. Analysis of the eclipses suggests i=84°.0±0°.8, q=0.155±0.015, M2=0.14±0.02 M☉, M1=0.90±0.13 M☉.:
Abstract Copyright: ∼
Journal keyword(s): accretion, accretion disks - Stars: Binaries: Close - Stars: Novae, Cataclysmic Variables - Stars: Individual: Constellation Name: DV Ursae Majoris
Simbad objects: 6
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