The infrared emission from supernova condensates

Details The infrared emission from supernova condensates The infrared emission from supernova condensates

Aug 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981apj...248..138d&link_type=abstract

Astrophysical Journal, Part 1, vol. 248, Aug. 15, 1981, p. 138-151.

Astronomy and Astrophysics

Astronomy

70

Emission Spectra, Infrared Astronomy, Interstellar Matter, Nebulae, Supernova Remnants, Cooling, Cosmic Dust, Crab Nebula, Ejecta, Grains, Infrared Telescopes

Scientific paper

The possibility of detecting grains formed in supernovae by observations of their emission in the infrared is examined. The basic processes determining the temperature and infrared radiation of grains in supernova environments are analyzed, and the results are used to estimate the infrared emission from the highly metal enriched fast moving knots in Cas A. The predicted fluxes lie within the reach of current ground-based facilities at 10 microns, and their emission should be detectable throughout the infrared band with cryogenic space telescopes.

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