Supernova Remnants and Nucleosynthesis (fos 30): CYCLE4-AUG-CARRYOVER

Details Supernova Remnants and Nucleosynthesis (fos 30): CYCLE4-AUG-CARRYOVER Supernova Remnants and Nucleosynthesis (fos 30): CYCLE4-AUG-CARRYOVER

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994hst..prop.5680d&link_type=abstract

HST Proposal ID #5680

Physics

Hst Proposal Id #5680 Interstellar Medium Sn &Amp, Snr

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. This program: FOS UV/optical spectra of two LMC remnants are to be obtained, following up on EARLY ACQ images from cycle 2. This program has been carried over from before the servicing mission in December 1993.

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