Titre du document

Structure of close binaries

Lien vers le document
Nom du Corpus

AstroConcepts

Auteur(s)
  • M. D. T. Naylor 1
  • S. P. S. Anand 1
Affiliation(s)
  • David Dunlap Observatory, University of Toronto, Richmond Hill, Ontario, Canada
Résumé

The stellar structure equations for uniformly rotating, synchronous close binaries have been derived using a modified double approximation technique which has been successful in studies of rotating stars and close binary polytropes. The auxiliary functions which are necessary to obtain interior models have been derived and their numerical values are given for various mass ratios. In order to calculate the apparent luminosities and colours of binary models the effects of gravity darkening (either radiative or convective) must be taken into account. Tables are presented for different degrees of distortion, mass ratio, and the two extremes of inclination which allow the apparent luminosity and mean effective temperature to be determined if the interior luminosity and separation of the components are given.

Langue(s) du document
Anglais
Année de publication
1972
Revue

Astrophysics and Space Science

Éditeur
Springer (journals)
Type de publication
journal
Type de document
research-article
Présence de XML structuré
Non
Version de PDF
1.3
Score de qualité du texte
7.67
Nom du concept
  • Roche equipotentials
Catégories Science-Metrix
  • 1 - natural sciences ; 2 - physics & astronomy ; 3 - astronomy & astrophysics
Catégories Inist
  • 1 - sciences appliquees, technologies et medecines ; 2 - sciences exactes et technologie ; 3 - terre, ocean, espace ; 4 - geophysique externe
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
2ABABED9A5D52687D8BC5F786C5BFC70317A67EB
ark:/67375/1BB-QNCXJJZJ-V
Powered by Lodex 9.4.5