Masses of Pre-Main Sequence Binaries

Details Masses of Pre-Main Sequence Binaries Masses of Pre-Main Sequence Binaries

Jul 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000hst..prop.8616s&link_type=abstract

HST Proposal ID #8616

Physics

Hst Proposal Id #8616 Cool Stars

Scientific paper

We propose to continue to map the orbits of young star binaries in the
Taurus and Ophiuchus star forming regions. Our goal is to measure their
masses dynamically. This is important because there are still no low
mass young stars with reliably known masses so calculations of their
evolution to the main sequence are uncalibrated.

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