A digital technique for the separation of the eclipses of a white dwarf and an accretion disc

Details A digital technique for the separation of the eclipses of a white dwarf and an accretion disc A digital technique for the separation of the eclipses of a white dwarf and an accretion disc

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985mnras.214..475w&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 214, June 1, 1985, p. 475-479. Research supported by th

Astronomy and Astrophysics

Astronomy

38

Accretion Disks, Cataclysmic Variables, Eclipsing Binary Stars, Light Curve, White Dwarf Stars, Data Processing, Digital Techniques, Temporal Distribution

Scientific paper

A method of extracting the white-dwarf component of an eclipse from the
light curve of an eclipsing cataclysmic variable is presented. The
method also gives the times of ingress and egress of the white dwarf and
the times of mid-eclipse.

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