Two-colour photometry and analysis of the eclipsing binary IM Aurigae

Details Two-colour photometry and analysis of the eclipsing binary IM Aurigae Two-colour photometry and analysis of the eclipsing binary IM Aurigae

Publishing date

Jun 1985

URL

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26as...60..389g&link_type=abstract

Journals

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 60, June 1985, p. 389-397. Sponsorship: Scientific and Techn

Science

Statistics

Field

Computation

Additional info 2

6

Additional info 3

Eclipsing Binary Stars, Electrophotometry, Light Curve, Stellar Spectrophotometry, Variable Stars, Computational Astrophysics, Orbital Elements, Radial Velocity, Roche Limit, Stellar Structure, Subgiant Stars

Type

Scientific paper

Abstract

Photoelectric observations of the eclipsing binary IM Aur have been carried out in B and V colours at the Ege University Observatory. The light curves were analyzed by means of Wood's model simulation program WINK and the Wilson-Devinney computer code. The system was found to be a detached binary with an undersized subgiant secondary nearly filling its Roche limit. The absolute elements of the system are also deduced.

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