Orbital Parameter of Known Binary, Sequel - Fixed

Details Orbital Parameter of Known Binary, Sequel - Fixed Orbital Parameter of Known Binary, Sequel - Fixed

Jul 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995hst..prop.6240j&link_type=abstract

HST Proposal ID #6240

Astronomy and Astrophysics

Astrophysics

Hst Proposal Id #6240 Stellar Astrophysics

Scientific paper

We propose to use FGS in TRANS mode to observe the close known binary ADS11300. According to an orbital analysis incorporating recent HST-FGS results, this pair of 54-yr orbital period is expected to pass through periastron in 1996.25 +/- 0.75 and will reach a component separation of 10 mas. The proposed observations, in combination with two observations to be secured in Cycle 6, will provide a critical test of the angular-resolution limits achievable with FGS in the TRANS mode.

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