The evolution of the line intensity ratios for supernova remnants in the Galaxy and in the Large Magellanic Cloud

Details The evolution of the line intensity ratios for supernova remnants in the Galaxy and in the Large Magellanic Cloud The evolution of the line intensity ratios for supernova remnants in the Galaxy and in the Large Magellanic Cloud

Dec 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976a%26a....53..443d&link_type=abstract

Astronomy and Astrophysics, vol. 53, no. 3, Dec. 1976, p. 443-445. Research supported by the Consiglio Nazionale delle Ricerche

Astronomy and Astrophysics

Astrophysics

16

Abundance, Galactic Evolution, Line Spectra, Magellanic Clouds, Milky Way Galaxy, Supernova Remnants, H Alpha Line, Spectral Energy Distribution

Scientific paper

Abstract image available at:
http://adsabs.harvard.edu/abs/1976A&A....53..443D

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