Mass Exchange Binaries (fos 34) SS 2883 : Cycle 4

Details Mass Exchange Binaries (fos 34) SS 2883 : Cycle 4 Mass Exchange Binaries (fos 34) SS 2883 : Cycle 4

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994hst..prop.5133m&link_type=abstract

HST Proposal ID #5133

Astronomy and Astrophysics

Astrophysics

Hst Proposal Id #5133 Stellar Astrophysics

Scientific paper

FOS UV spectroscopy will be used to study the Be star (SS 2883; CD-63D2495) binary companion to the pulsar PSR1259-63. The pulsar is eclipsed near periastron, due to the wind of the Be star, and or a circumstellar disk. UV spectra near periastron will be used to probe the Be star wind and disk material, and perhaps their interaction with the pulsar.

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