The orbital elements and physical properties of the eclipsing binary BD+36°3317, a probable member of δ Lyrae cluster
Articles > Article · 2016
Authors: E. Kıran, P. Harmanec, Ö. L. Değirmenci, M. Wolf, J. Nemravová, M. Šlechta, P. Koubský
Astronomy & Astrophysics, International, WoS, 2016, vol 587, pp A127-A127
DOI: 10.1051/0004-6361/201527211
Summary
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.