Stellar Wind Variations -- Cycle 1

Details Stellar Wind Variations -- Cycle 1 Stellar Wind Variations -- Cycle 1

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991hst..prop.1152h&link_type=abstract

HST Proposal ID #1152

Physics

Hst Proposal Id #1152

Scientific paper

UV spectroscopy will be done at 2 x 10super4 resolution on the principal stellar wind lines of OB stars with mass-loss. Each star will be observed twice to study time changes in line profiles. Several stars are interacting binaries. These will also be observed at key binary phases to study phase dependent wind variations. WFC parallel observations with UV grating are requested on one SMC star.

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