Determination of the parameters of the eclipsing binary system V367 CYG by the light-curve synthesis method

Details Determination of the parameters of the eclipsing binary system V367 CYG by the light-curve synthesis method Determination of the parameters of the eclipsing binary system V367 CYG by the light-curve synthesis method

Jun 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990pazh...16..539a&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 16, June 1990, p. 530-538. In Russian. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

Eclipsing Binary Stars, Independent Variables, Light Curve, Roche Limit, Stellar Models, Cygnus Constellation, Mass Spectroscopy

Scientific paper

Fresa's (1966) blue light curve of V367 Cyg is analyzed by the synthesis
method in the framework of the Roche model and a model with a
geometrically thick disk. The new spectroscopic mass ratio q = M2//M1 =
1.57 was used. The fundamental parameters and the absolute dimensions of
the system were determined.

Affiliated with

Also associated with

No associations

Rating

Determination of the parameters of the eclipsing binary system V367 CYG by the light-curve synthesis method 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 Determination of the parameters of the eclipsing binary system V367 CYG by the light-curve synthesis method, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Determination of the parameters of the eclipsing binary system V367 CYG by the light-curve synthesis method will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-988521