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MPIfR Optical & Infrared Interferometry Group


A.A. Tokovinin, Y.Y. Balega, K.-H. Hofmann, and G. Weigelt:

The orbit of the nearby low-mass binary Gliese 600

Astronomy Letters 26, 668-671 (2000)


Abstract. We have computed a combined spectroscopic-interferometric orbit for the nearby binary Gliese 600 discovered by us. The orbital period is 2.78 years, and the semimajor axis is 100 mas (0.1"). Its M0 V components are almost identical and have a mass of 0.5M. The mass ratio is uncertain because of the low radial-velocity semiamplitude (7 km/s) associated with the low orbital inclination (37°). The orbital parallax of the binary (52 ± 11 mas) matches its dynamical and photometric parallaxes but differs significantly from the Hipparcos parallax (44.3 ± 1.6) mas; the latter was probably distorted by the orbital motion that was not taken into account.

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