Mass Exchange Binaries (fos 34) -- Cycle 0

Details Mass Exchange Binaries (fos 34) -- Cycle 0 Mass Exchange Binaries (fos 34) -- Cycle 0

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990hst..prop.1051m&link_type=abstract

HST Proposal ID #1051

Computer Science

Hst Proposal Id #1051

Scientific paper

FOS UV spectra will be used to probe the effect of ionizing radiation from the compact star on the atmosphere of the normal companion, gaining information on the unobservable soft X-ray spectrum of the system which may, in some cases, dominate the energy budget. The FOS time resolved mode permits data also to be obtained as a function of pulse phase for X-ray pulsars, especially in the UV, where the strong resonance lines are available, and the FOS polarimeter will be used to examine the orbital phase dependence of polarization in these lines in the polars, providing new data on the complex structure of the accretion column.

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