Photometric study of the eclipsing binary V1034 Sco
Astronomy Group, Vrije Universiteit Brussels (VUB), Pleinlaan 2, 1050 Brussels, Belgium e-mail: [ybouzid;csterken]@vub.ac.be
2 Astronomical Institute of the Slovak Academy of Sciences, 05960 Tatranská Lomnica, The Slovak Republic e-mail: email@example.com
Accepted: 14 March 2005
We present multi-colour Strömgren photometry of the eclipsing binary V1034 Sco in the galactic open cluster NGC 6231, providing for the first time a full coverage of the orbital period ( days) and a complete analysis of the orbit. This extensive new photometry was analyzed together with multiband spectroscopy and results in an improved ephemeris, photometric elements and absolute parameters of the components. The system is close, but clearly detached. The masses of the components and do not correspond to the published spectral classification (O9III + B1III). The parameters of the components are consistent with the main-sequence luminosity class. We independently derive a distance modulus .
Key words: instrumentation: photometers / binaries: eclipsing / methods: data analysis / methods: observational / techniques: photometric / Hertzspring-Russell and C-M diagrams
© ESO, 2005