Orbits of Pre-Main Sequence Binaries

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

Dec 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997hst..prop.7487s&link_type=abstract

HST Proposal ID #7487

Physics

Hst Proposal Id #7487 Young Stars And Circumstellar Material

Scientific paper

Our goal is to measure the masses of low mass pre-main sequence stars dynamically. This is important because there are still no low mass young stars with reliably known masses. We have begun to map the orbits of young star binaries in Taurus using the FGS. We propose to continue to measure the orbits of the systems we have determined to have the smallest angular separations. These may be expected to have the shortest periods and are uniquely observable by the HST.

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