The physical parameters and orbit of the eclipsing binary system GSC 4596 1254 = SAO 3282 View Full Text


Ontology type: schema:ScholarlyArticle     


Article Info

DATE

2009-02

AUTHORS

I. M. Volkov, N. S. Volkova

ABSTRACT

We have obtained the first U BV R photoelectric light curves for a recently discovered eclipsing binary with a period of 9.33d and an appreciable eccentricity (e = 0.08). We have used these data to determine the photometric elements of the system for a model with two spherical stars with linear limb darkening. The high accuracy of the observations enabled determination of the absolute parameters of the components using available calibrations. The masses of the components are 1.28 and 1.08 M⊙, and their ages are two billion years. The present orientation of the orbital ellipse is unfavorable for studies of the apsidal rotation, which is essentially due to relativistic effects. More... »

PAGES

136-147

Journal

TITLE

Astronomy Reports

ISSUE

2

VOLUME

53

Author Affiliations

Identifiers

URI

http://scigraph.springernature.com/pub.10.1134/s106377290902005x

DOI

http://dx.doi.org/10.1134/s106377290902005x

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1034240417


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