Absolute Parameters of the O-type Eclipsing Binary V 1007 Sco

Details Absolute Parameters of the O-type Eclipsing Binary V 1007 Sco Absolute Parameters of the O-type Eclipsing Binary V 1007 Sco

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007iaus..240..326n&link_type=abstract

Binary Stars as Critical Tools and Tests in Contemporary Astrophysics, International Astronomical Union. Symposium no. 240, he

Astronomy and Astrophysics

Astrophysics

Scientific paper

A definitive set of orbital and physical parameters of the binary system V 1007 Sco is presented. Both stars are classified as O7 giants. Light and RV curves were simultaneously analyzed with PHOEBE, a modern WD-based solution code. A statistical approach yielded realistic error estimates. Orbital eccentricity is 0.12 with an apsidal motion period of 112 years.

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