Binary Stars behind the Vela Super Nova Remnant

Details Binary Stars behind the Vela Super Nova Remnant Binary Stars behind the Vela Super Nova Remnant

Jul 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999hst..prop.8045d&link_type=abstract

HST Proposal ID #8045

Computer Science

Hst Proposal Id #8045 Interstellar Matter

Scientific paper

Spectroscopic observations of a pair of double stars behind the Vela SNR, in the UV provide information on the variations of the intersteallar medium composition, spatially and because these stars have been observed earlier by GHRS the data will also provide a measure of temporal variations. The Vela SNR is close and movement of the ISM infront perpendicular to the sightline is easily seen. Observations of interstellar lines and line ratios will give information on shock scale lengths and grain destruction.

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