A standard accretion disc model for RW Tri

Details A standard accretion disc model for RW Tri A standard accretion disc model for RW Tri

Apr 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981mnras.195..227f&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 195, Apr. 1981, p. 227-234.

Astronomy and Astrophysics

Astronomy

24

Dwarf Stars, Eclipsing Binary Stars, Infrared Astronomy, Light Curve, Novae, Stellar Mass Accretion, Companion Stars, Stellar Magnitude, Stellar Mass, Stellar Models, Stellar Occultation

Scientific paper

The infrared and visual light curves of the cataclysmic binary RW Tri
during quiescence are simultaneously fitted by a model in which a red
dwarf secondary eclipses an optically thick steady-state accretion disk.
This enables the estimation of self-consistent parameters for this
model.

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