Infrared emission from the supernova remnant Puppis A: dust and gas parameters.

Details Infrared emission from the supernova remnant Puppis A: dust and gas parameters. Infrared emission from the supernova remnant Puppis A: dust and gas parameters.

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989iaus..135p.543a&link_type=abstract

IAU Symposium No. 135: Interstellar dust: contributed papers, p. 543 - 548

Computer Science

Supernova Remnants: Infrared Radiation, Supernova Remnants: Gas Densities, Supernova Remnants: Temperatures

Scientific paper

The authors have modelled the infrared spectra of collisionally heated dust at several regions across the supernova remnant Puppis A. Through the comparison of the actual and model spectra, they are able to narrow the possible range of gas density and temperature within these areas. From the models, they also find information on the minimum and maximum dust grain sizes, and the amount of sputtering which has occurred.

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