Supernova Remnants and Nucleosynthesis (fos 30): CYC3-AUG-HIGH

Details Supernova Remnants and Nucleosynthesis (fos 30): CYC3-AUG-HIGH Supernova Remnants and Nucleosynthesis (fos 30): CYC3-AUG-HIGH

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993hst..prop.4860d&link_type=abstract

HST Proposal ID #4860

Physics

Hst Proposal Id #4860

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. In earlier parts of the program, an oxygen-rich SNR in NGC 4449 was 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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