C. Barbieri et al., FIRST HST FOC IMAGES OF THE LOW-MASS COMPANION OF THE ASTROMETRIC BINARY GLIESE-623/, Astronomy and astrophysics, 315(3), 1996, pp. 418-420
We have resolved the astrometric binary Gliese 623 into two components
, by direct imaging in the visible band, with the COSTAR corrected FOG
. The images clearly show the faint companion Gliese 623B, with a deri
ved absolute magnitude of M(V) = 16.17 +/- 0.10, at a distance of 0.33
'' from the primary (namely at 2.51 AU, assuming a parallax of pi = 0
''.132, i.e. a distance of 7.6 pc). From the mass-luminosity relation
ship of Henry and McCarthy (1993), the photometric mass of the seconda
ry is 0.098 solar masses.