Supernova Remnants and Nucleosynthesis (fos 30) - Cycle 1

Details Supernova Remnants and Nucleosynthesis (fos 30) - Cycle 1 Supernova Remnants and Nucleosynthesis (fos 30) - Cycle 1

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991hst..prop.3205d&link_type=abstract

HST Proposal ID #3205

Physics

Hst Proposal Id #3205

Scientific paper

UV and optical spectra of six 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. Two SNRs in M33 will be observed to study abundances and abundance gradients of elements not readily available from optical spectra and that are too faint for IUE. 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.

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