Optical supernova remnants in external galaxies

Details Optical supernova remnants in external galaxies Optical supernova remnants in external galaxies

Nov 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982sscr.conf..483d&link_type=abstract

In: Supernovae: A survey of current research; Proceedings of the Advanced Study Institute, Cambridge, England, June 29-July 10,

Astronomy and Astrophysics

Astronomy

4

Astronomical Spectroscopy, Optical Emission Spectroscopy, Supernova Remnants, Abundance, Balmer Series, Galaxies, Line Spectra, Stellar Evolution, Visible Spectrum

Scientific paper

Optical emission observations of SNRs first identified on the basis of their X-ray properties by HEAO 2 have revealed several examples of unusual classes of objects which would have evaded identification by means of classical criteria. Results are given from an optical survey conducted at Mt. Stromlo, which has detected young remnants of Type II events, remnants of Type I events, and phenomena relevant to the evolution of old SNRs. Attention is given to abundance-sensitive line ratios in external galaxy SNRs, the galactic abundance gradient, and nonequilibrium conditions in SNRs.

Affiliated with

Also associated with

No associations

Rating

Optical supernova remnants in external galaxies does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Optical supernova remnants in external galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Optical supernova remnants in external galaxies will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1759200