Titre du document

SV Cam, an eclipsing binary containing a BY Draconis variable

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Nom du Corpus

AstroConcepts

Auteur(s)
  • R. W. Hilditch 1
  • D. M. Harland 2
  • B. J. McLean 3
Affiliation(s)
  • University Observatory, St Andrews, Scotland
  • Department of Computational Science, University of St Andrews
  • University Observatory, St Andrews Communicated by the Director, University Observatory, St Andrews
Résumé

New photometric observations are presented of the short-period eclipsing binary system SV Cam. These, together with published data, are analysed and it is shown that the system is composed of a G3 V primary component slightly evolved above the main sequence and a K4 V secondary component which also exhibits BY Draconis-type variability. The extensive series of published times of minima indicate that the eclipsing pair orbit a third component with a period of 64 yr.

Langue(s) du document
Indéterminé
Année de publication
1979
Revue

Monthly Notices of the Royal Astronomical Society

Éditeur
OUP
Type de publication
journal
Type de document
research-article
Présence de XML structuré
Non
Version de PDF
1.4
Score de qualité du texte
2.913
Nom du concept
  • BY Draconis stars
Catégories Science-Metrix
  • 1 - natural sciences ; 2 - physics & astronomy ; 3 - astronomy & astrophysics
Catégories Scopus
  • 1 - Physical Sciences ; 2 - Earth and Planetary Sciences ; 3 - Space and Planetary Science
  • 1 - Physical Sciences ; 2 - Physics and Astronomy ; 3 - Astronomy and Astrophysics
Catégories WoS
  • 1 - science ; 2 - astronomy & astrophysics
Identifiant ISTEX
193102A902FB0FC17AED117D216921BFF101CDD8
ark:/67375/HXZ-WF95NNMT-K
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