Orbits of Pre-Main Sequence Binaries

Details Orbits of Pre-Main Sequence Binaries Orbits of Pre-Main Sequence Binaries

Jul 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000hst..prop.8783s&link_type=abstract

HST Proposal ID #8783

Physics

Hst Proposal Id #8783

Scientific paper

Our goal is to dynamically measure the masses of low mass pre-main sequence stars. This is important because there are still no low mass young stars with reliably known masses. In cycle 5 we began to map the orbits of young multiple star systems in Taurus using FGS3. We propose to continue to measure the orbits of the binary and triple systems we have determined to have the smallest angular separations with the more capable FGS1r. These systems are expected to have the shortest periods and are uniquely observable by the HST.

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