The orbital elements and physical properties of the eclipsing binary BD+36 degrees 3317, a probable member of delta Lyrae cluster


Creative Commons License

Kiran E., Harmanec P., DEĞİRMENCİ Ö. L. , Wolf M., Nemravova J., Slechta M., ...More

ASTRONOMY & ASTROPHYSICS, vol.587, 2016 (Journal Indexed in SCI) identifier identifier

  • Publication Type: Article / Article
  • Volume: 587
  • Publication Date: 2016
  • Doi Number: 10.1051/0004-6361/201527211
  • Title of Journal : ASTRONOMY & ASTROPHYSICS
  • Keywords: binaries: eclipsing, stars: fundamental parameters, stars: individual: BD+36 degrees 3317, ASTROPHYSICAL SUPPLEMENTS, RADIAL-VELOCITIES, LIGHT CURVES, STARS, PARAMETERS, PHOTOMETRY, PLEIADES, ASCC-2.5

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.