Mass Exchange Binaries (fos 34) Augmentation: Cycle 3 - High

Details Mass Exchange Binaries (fos 34) Augmentation: Cycle 3 - High Mass Exchange Binaries (fos 34) Augmentation: Cycle 3 - High

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993hst..prop.4866m&link_type=abstract

HST Proposal ID #4866

Computer Science

Hst Proposal Id #4866

Scientific paper

The FOS GTO program includes a systematic study of degenerate stars in binary systems, both in the field and in globular clusters, plus a handful of related objects. For the isolated field systems, the emphasis is on spectro- photometry (in many cases time-resolved over a pulse or orbital period) and spectropolarimetry, to observe the effects of the intense ionizing flux emitted by the compact object on the nearby normal star and/or accretion disk. While some such effects are seen from the ground, they should be far more spectacular in the UV. The specific program in this proposal is UV spectropolarimetry of V1727-CYG.

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