THE LOWEST MASS STARS IN THE HYADES

In Bryja et al., [ApJ, 388, L23 (1992)], we presented proper motions a nd photometry of 12 very low mass star and brown dwarf candidates in t he Hyades cluster, selected on the basis of colors and proper motions measured from three epochs of plate material. We here present new obse rvations of some of these candidates, including seven low resolution s pectra, plus motions and photometry of 17 fainter additional candidate s. Most of the candidates have JHK colors typical of M5-M8 dwarfs, whi le their optical colors are consistent with earlier M spectral types. The available spectra consist of late M dwarfs with Ha emission featur es indicative of Hyades membership, earlier M dwarf background stars, and two anomalous objects with early M dwarf features but unusually re d continua. We find that the proper motion distribution of faint red f ield stars in the region is irregular, and it is not possible to deter mine if the anomalous objects are Hyades members or background field s tars. In the most conservative view, only five of our 29 candidates ar e Hyads. These five stars have optical and infrared colors consistent with the bottom of the Hyades main sequence, with four of them also sh own to have late M dwarf spectra. It follows that these are the lowest mass stars known in the Hyades (M approximately 0.1 M.).