Detection and Mass Determination of Low-Mass Companions to Nearby M Dwarfs

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Hst Proposal Id #6036 Cool Stars

Scientific paper

We observe GL791 9 times during Cycle 5. When added tothe 6 observations to be secured during Cycle 6, we will obtaina precise parallax and a relative orbit for a faint companion to this star.We observe GL275 in October 1995. If we detect the possiblefaint companion, we will secure 5 more observations in Cycle 5, ninemore in Cycle 6. Should the October 1995 observation not show any companion,we will observe GJ1081 5 times in Cycle 5, nine times in Cycle 6.The result will be a precise parallax and a relative orbit for a faintcompanion to this star.

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