Hubble Space Telescope observations of M subdwarfs

We present the results of a Hubble Space Telescope snapshot program to sear ch for very low mass stellar companions to nearby M subdwarfs. None of our nine targetted metal-poor primaries has companions more massive than the hy drogen burning limit, implying that the halo binary fraction is equal to or less than the Galactic disk binary fraction below 0.3 M.. In addition, the more distant tertiary VB 12, an sdM3.0 companion to an F subdwarf double, is also unresolved. We show that the relation between WFPC2 F555W and F850L P photometry and ground-based V, I photometry is consistent with theoretica l expectations. We also report that two recently observed Hyades M dwarfs a ppear single.