Photometry of the eclipsing cataclysmic variable NSV 12615

Details Photometry of the eclipsing cataclysmic variable NSV 12615 Photometry of the eclipsing cataclysmic variable NSV 12615

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989mnras.241..631b&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 241, Dec. 15, 1989, p. 631-644.

Other

18

Cataclysmic Variables, Eclipsing Binary Stars, Stellar Mass Accretion, Stellar Spectrophotometry, Accretion Disks, Astronomical Photometry, Light Curve, Starspots, Stellar Luminosity, White Dwarf Stars

Scientific paper

A photometric study of NSV 12615 based on 25 eclipses observed during the last four years is presented. A range of values is obtained for the component masses, the orbital inclination, and other system parameters. The high relative brightness of the disk as compared to the white dwarf plus bright spot could be a consequence of a high accretion rate. The differences between this system and other short-period eclipsing cataclysmic variables are discussed.

Affiliated with

Also associated with

No associations

Rating

Photometry of the eclipsing cataclysmic variable NSV 12615 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Photometry of the eclipsing cataclysmic variable NSV 12615, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Photometry of the eclipsing cataclysmic variable NSV 12615 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1575433