Supernova Remnants and Nucleosynthesis (fos 30): Cycle 2 Baseline Observations

Details Supernova Remnants and Nucleosynthesis (fos 30): Cycle 2 Baseline Observations Supernova Remnants and Nucleosynthesis (fos 30): Cycle 2 Baseline Observations

Jul 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992hst..prop.3296d&link_type=abstract

HST Proposal ID #3296

Physics

Hst Proposal Id #3296

Scientific paper

Overall program: UV and optical spectra of four supernova remnants (SNRs) will be used to study a number of problems related to abundances, grain destruction, interstellar medium properties and physical conditions in SNR shocks. Representatives of three of the main classes of SNRs (Crab-nebula like, Balmer-line and "normal") will be studied in the LMC, where reasonably low reddening permits UV observations. An oxygen-rich SNR in NGC 4449 will be observed, taking advantage of the small FOS slits to isolate the SNR from surrounding H II emission. Two M33 SNRs that were previously part of this proposal have been dropped due to time limitations.

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