The massive WC6+O6-8 spectroscopic binary HD 94305

Details The massive WC6+O6-8 spectroscopic binary HD 94305 The massive WC6+O6-8 spectroscopic binary HD 94305

Sep 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983apj...272..190n&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 272, Sept. 1, 1983, p. 190-195. Research supported by the Natural Sciences

Astronomy and Astrophysics

Astrophysics

14

Binary Stars, Carbon Stars, Radial Velocity, Stellar Mass, Stellar Spectra, Wolf-Rayet Stars, O Stars, Orbital Elements, Stellar Evolution

Scientific paper

HD 94305 is found to be a double-lined WC6+O6-8 spectroscopic binary. The minimum masses of the components of this binary are 15 and 32 solar mass for the Wolf-Rayet and the O type components, respectively. The relatively high minimum mass for the WC6 component adds further evidence to the notion presented elsewhere by Niemela (1981) that the more massive WC6-8 stars cannot be descendants of the less massive WN3-5 stars.

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