Calibrating the Mass-Luminosity Relation at the End of the Main Sequence

Details Calibrating the Mass-Luminosity Relation at the End of the Main Sequence Calibrating the Mass-Luminosity Relation at the End of the Main Sequence

Jul 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995hst..prop.6047h&link_type=abstract

HST Proposal ID #6047

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Hst Proposal Id #6047 Cool Stars

Scientific paper

We observe GL748 9 times during Cycle 5. When added to the 6 observations to be secured during Cycle 6, we will obtain a precise parallax and a relative orbit for a faint companion to this star. The other targets are observed in TRANS mode to detect faint companions. In some cases {GL 1245, GL 22, GL 473, GL234} the expected orbital motion is large enough to warrant two observations in Cycle 5.

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