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2000PASP..112.1269T - Publ. Astron. Soc. Pac., 112, 1269-1276 (2000/September-0)
Spectroscopy and component masses of the eclipsing dwarf nova HS 0907+1902.
THORSTENSEN J.R.
Abstract (from CDS):
The Hα emission-line profile out of eclipse is only slightly double-peaked, but the line shows a strong rotational disturbance in eclipse. Models of the line profile through eclipse using a flat, Keplerian disk do not give a good quantitative match to the observations.
Abstract Copyright: ∼
Journal keyword(s): Stars: Binaries: Eclipsing - Stars: Binaries: Spectroscopic - Stars: Novae, Cataclysmic Variables - Stars: Fundamental Parameters - stars: individual (HS 0907+1902) - Stars: White Dwarfs
Simbad objects: 4
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