LMC X-Ray Sources

Details LMC X-Ray Sources LMC X-Ray Sources

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991hst..prop.1151h&link_type=abstract

HST Proposal ID #1151

Physics

Hst Proposal Id #1151

Scientific paper

FOS high and low dispersion spectra wil be obtained in the UV to study stellar wind lines at selected orbital phases. In LMC X-4, these will be carried out at two precessional phases as well. The data will be used to study stellar wind ionisation and velocity changes with X-ray binary phase, and with variable accretion disk obscuration of X-rays. WFC images with UV grating and UV filter in parallel to study LMC hot star population.

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