Astronomy and Astrophysics – Astrophysics
Scientific paper
Mar 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26a...174....5c&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 174, no. 1-2, March 1987, p. 5-12.
Astronomy and Astrophysics
Astrophysics
5
Astronomical Models, Magellanic Clouds, Shock Waves, Supernova Remnants, Ejecta, Helium, Infrared Radiation, Nitrogen, Oxygen, Radio Emission, Visible Spectrum
Scientific paper
Observational data on SNRs are analyzed in terms of the interaction between SNRs and the interstellar medium (ISM) and the physical processes related to the SNR phenomena. Examples of the interaction of SNRs with the local ISM are presented. The origin and decay of radiation in the different spectral regions are examined. The physical conditions in the SNRs of the LMC are investigated by fitting calculated optical spectra to the spectra of Danziger and Leibowitz (1985). The nonequilibrium ionization model of Contini et al. (1980) and Contini and Aldrovandi (1983 ) was utilized for the calculation of the spectra. It is noted that the interaction of the shock front with clouds of different densities affects the physical conditions inside some of the observed objects in the LMC.
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