Delta Capricorni - an evolved binary or a main-sequence binary?

Details Delta Capricorni - an evolved binary or a main-sequence binary? Delta Capricorni - an evolved binary or a main-sequence binary?

Feb 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989aj.....97..499m&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 97, Feb. 1989, p. 499-504. Research supported by the Japan Society for the Promotion

Astronomy and Astrophysics

Astronomy

4

Eclipsing Binary Stars, Main Sequence Stars, Peculiar Stars, Stellar Spectrophotometry, F Stars, Light Curve, Light Scattering

Scientific paper

A synthesis method is used to analyze B and V observations of Delta Cap obtained at the Bosscha Observatory in 1984 and 1985. Both components of the binary are found to be well inside their critical Roche lobes. The data are consistent with a model using a mass radio q = 0.365 which yields a main-sequence mass for the primary star. A distance of 8-11 pc is implied.

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