Absolute dimensions of eclipsing binaries. XXV. U Ophiuchi and the evolution and composition of 5 M⊙ stars
Abstract
Context: Precise stellar masses and radii provide unique information on stellar evolution. In a Galactic context, they may also provide information on the evolution of the Solar neighbourhood.
Aims: We aim to determine absolute dimensions for the mid B-type eclipsing binary U Ophiuchi and compare the inferred ages and chemical compositions to those of other binary stars with masses near 5 {M}⊙.
Methods: We determine masses, radii, log g, log T_eff, and luminosities for the stars in U Oph from new radial velocities and uvby light curves. By improving the Wilson-Devinney code, we also derive precise apsidal-motion and light-time orbits of this triple system, using 353 times of minimum over 120 years. Finally, we compare the data for U Oph and three similar systems with the predictions of stellar models.
Results: The stars in U Oph have masses of 5.27 ± 0.09 {M}⊙ and 4.74 ± 0.07 {M}⊙, radii of 3.48 ± 0.02 {R}⊙ and 3.11 ± 0.03 {R}⊙; we argue that systematic errors are negligible. The apsidal motion period is exceptionally short, U ∼21 yr, while the light-time orbit has P3 ∼ 38.4 yr. The precise log g values for
Conclusions: More accurate data and/or binary systems with larger mass ratios are needed to actually test stellar models near 5 {M}⊙. The different Z values found for these young, nearby systems suggest that disk stars form with a range of metal abundances even today, but more data are needed to confirm this result.
- Publication:
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Astronomy and Astrophysics
- Pub Date:
- July 2007
- DOI:
- 10.1051/0004-6361:20066911
- Bibcode:
- 2007A&A...469..285V
- Keywords:
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- stars: binaries: eclipsing;
- stars: fundamental;
- parameters;
- stars: evolution;
- Galaxy: evolution