The orbital elements and physical properties of the eclipsing binary BD+36°3317, a probable member of<i>δ</i>Lyrae cluster

Evrim Kıran, P. Harmanec, Ö. L. Değirmenci, M. Wolf, J. Nemravová, M. Šlechta, P. Koubský

Type: Article

Publication Date: 2016-01-08

Citations: 2

DOI: https://doi.org/10.1051/0004-6361/201527211

Abstract

Context. The fact that eclipsing binaries belong to a stellar group is useful, because the former can be used to estimate distance and additional properties of the latter, and vice versa.

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