Masses of Premain Sequence Stars CYC4MEDIUM

Details Masses of Premain Sequence Stars CYC4MEDIUM Masses of Premain Sequence Stars CYC4MEDIUM

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994hst..prop.5316s&link_type=abstract

HST Proposal ID #5316

Physics

Hst Proposal Id #5316 Cool Stars Early Evolution

Scientific paper

We propose to determine the masses of pre-main sequence binaries selected from our lunar occultation survey of the Taurus star-forming region. We plan to use the Fine Guidance Sensors to measure the apparent orbits of the binaries. Since the distance to the region is known the apparent orbits will yield the total masses of the binaries. This proposal is for the third year continuation for our program previously approved for Cycles 2 and 3. No data has been taken yet so we can only summarize our goals and plans. The first observations are scheduled for September and October 1993. We will use those results to update the target list as described in Question 4.

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