Rediscussion of eclipsing binaries. XIV - The bright AM system V624 Herculis

Details Rediscussion of eclipsing binaries. XIV - The bright AM system V624 Herculis Rediscussion of eclipsing binaries. XIV - The bright AM system V624 Herculis

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984aj.....89.1057p&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 89, July 1984, p. 1057-1062. NSF-supported research.

Astronomy and Astrophysics

Astronomy

14

A Stars, Eclipsing Binary Stars, Metallic Stars, Peculiar Stars, Light Curve, Radial Velocity, Spectrograms

Scientific paper

V624 Her is a 6th magnitude 3d.6 double-lined eclipsing metallic-lined binary of middle A type with eclipses about 0.18 mag deep. Analysis of a new set of 6.7 Å mm-1 spectrograms, combined with a reanalysis of Zissell's curve on the basis of the spectrophotometric light ratio, yields well-determined properties of the components. The hotter component is the most massive and the largest of all Am stars with well-determined properties.

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