Computer Science
Scientific paper
Jul 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993hst..prop.4868b&link_type=abstract
HST Proposal ID #4868
Computer Science
Hst Proposal Id #4868
Scientific paper
Two interacting binaries with accretion disks have been selected to determine the nature of the stellar components, and mass flow characteristics of the systems. These objects are the well-known x-ray binaries Sco X-1 and HZ Her. GHRS observations with the medium resolution G160M grating will be used to provide superior signal-to-noise and resolution than presently available using IUE.
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