Duplicity among Hyades Stars Cycle 3, High

Details Duplicity among Hyades Stars Cycle 3, High Duplicity among Hyades Stars Cycle 3, High

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993hst..prop.4892j&link_type=abstract

HST Proposal ID #4892

Computer Science

Hst Proposal Id #4892

Scientific paper

We propose to use FGS in the TRANS mode to examine, at high angular resolution, a representative sample of probable Hyades cluster members in an effort to establish the incidence of duplicity among Hyades stars. The frequency of multiple stars in stellar systems and populations represents a significant aspect of star formation and stellar evolution. Among Hyades stars brighter than V ~ 12.0, companions should be observable to Delta m ~ 2. Binaries of small Delta m should be readily detectable at V ~ 15.

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