Geometrical and physical elements of four Beta Lyrae type eclipsing variables

Details Geometrical and physical elements of four Beta Lyrae type eclipsing variables Geometrical and physical elements of four Beta Lyrae type eclipsing variables

Dec 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.117..351a&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 117, no. 2, Dec. 1985, p. 351-361.

Astronomy and Astrophysics

Astrophysics

2

Eclipsing Binary Stars, Variable Stars, Fourier Analysis, Hertzsprung-Russell Diagram, Light Curve

Scientific paper

The aim of the present paper is to present the analysis of light changes of four β Lyrae eclipsing systems (DO Cas, KR Cyg, V388 Cyg, and SV Cen) using the automated Fourier techniques in the frequency-domain. The applicability of the above method to the β Lyrae system is discussed. New physical and geometrical elements of these systems are derived. Their positions in the H-R diagram and mass-luminosity diagram are indicated.

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