Astronomy and Astrophysics – Astrophysics
Scientific paper
Sep 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...236..399l&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 236, no. 2, Sept. 1990, p. 399-408.
Astronomy and Astrophysics
Astrophysics
25
Binary Stars, M Stars, Stellar Composition, Stellar Mass, Stellar Orbits, Stellar Temperature, Dwarf Stars, Hertzsprung-Russell Diagram, Speckle Interferometry, Stellar Atmospheres, Stellar Luminosity, Stellar Spectra
Scientific paper
The relative orbit of the nearby M dwarf binary Gliese 866 has been determined from IR speckle interferometric observations. The true semimajor axis of 0.36 + or - 0.01 arcsec corresponds, for the distance of 3.4 pc and the period of 2.20 + or - 0.02 years, to a system mass of 0.38 + or - 0.02 solar masses. This is higher than expected on the basis of the systems's luminosity. The brightness ratio of the components is virtually constant at 0.56 + or - 0.04 in the near-IR, suggesting that both are of nearly the same spectral type. Comparison of coude spectra with newly developed model atmospheres for cool dwarf stars indicates element abundances close to solar values and effective temperatures of 2900 + or - 100 K for the primary and 2500-2750 K for the companion. For this system therefore all important physical parameters are determined with good reliability.
Allard France
Haas Marcel
Jahreiss Hartmut
Leinert Ch.
McCarthy Donald W.
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