Photometric Solution of the O-type Eclipsing Binary V1007 Sco

Details Photometric Solution of the O-type Eclipsing Binary V1007 Sco Photometric Solution of the O-type Eclipsing Binary V1007 Sco

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ap%26ss.304...47n&link_type=abstract

Astrophysics and Space Science, Volume 304, Issue 1-4, pp. 47-49

Astronomy and Astrophysics

Astrophysics

V1007 Sco, O-Type Binaries, Eccentric

Scientific paper

Improved orbital and physical parameters of the eccentric O-type system V1007 Sco (P=5.8 days) are presented. UBV light curves obtained over a period of 12 years were analyzed with a Wilson-Devinney-based solution code. Setting off from a set of parameters derived from spectroscopic investigations a consistent photometric solution was achieved. In accordance with the spectroscopic findings the eccentricity was determined as e=0.128 and the apsidal motion with a spectroscopic period of about 150 days was confirmed.

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