What is the mass ratio of the binary system RW Tri?

Details What is the mass ratio of the binary system RW Tri? What is the mass ratio of the binary system RW Tri?

Jan 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aspc..261...67p&link_type=abstract

The Physics of Cataclysmic Variables and Related Objects, ASP Conference Proceedings, Vol. 261. Edited by B. T. Gänsicke, K. Beu

Physics

Scientific paper

The eclipsing disc accreting CV RW Tri is one of the brightest known novalike variables, but the masses of the component stars are still poorly constrained. Results from a study of RW Tri in the near infrared and infrared constrain the secondary star velocity to 200 km/s (accurate to 10%). Combining this with optical and ultraviolet data for the primary star gives a range of mass ratios (M2 / M1) of 0.9--1.5.

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