Masses and Distances of Pre-Main Sequence Binaries

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

Jul 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999hst..prop.8319s&link_type=abstract

HST Proposal ID #8319

Physics

Hst Proposal Id #8319 Young Stars And Circumstellar Material

Scientific paper

We propose the continuation of FGS measurements of the orbital motion of young stars successfully carried out in Cycle 7 and earlier cycles. We need to continue these observations to acquire sufficient data to determine the orbital parameters of the binaries. Our goal is to measure the masses of low mass young stars. This will enable a calibration of theoretical calculations of stellar evolution to the main sequence.

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