Published July 15, 1973 | Version v1
Journal article Metadata-only

Stellar masses derived from the binary HD 217312

Creators

  • 1. David Dunlap Observatory, University of Toronto, Richmond Hill, Ontario, Canada

Description

It is shown that the component stars of the binary HD 217312 have masses of 27 I 2 and 13 I 1 . The absolute bolometric magnitudes of the two stars are -6.2 I 0.4 and -5.2 + 0 4 respectively. Subject headitigs: associations - eclipsing binaries - mass-luminosity relation - stars, individual

Additional details

Additional titles

Augmented title (English)
Eclipsing system, absolute bolometric magnitudes

Identifiers

DOI
10.1086/152248;

Publishing Information

Journal Title
The Astrophysical Journal
Journal Volume
183
Journal Issue
2
Series
Astrophys. J.
Journal Page Range
583
ISSN
0004-637X

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
5123397
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
ABSORPTION; BINARY STARS; LUMINOSITY; MASS; REFLECTION
Descriptors DEC
OPTICAL PROPERTIES; PHYSICAL PROPERTIES; STARS

Optional Information

Notes
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