Infrared emission from interstellar grains heated by supernovae

Details Infrared emission from interstellar grains heated by supernovae Infrared emission from interstellar grains heated by supernovae

Oct 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ap%26ss..96..159p&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 96, no. 1, Oct. 1983, p. 159-170.

Astronomy and Astrophysics

Astronomy

3

Far Infrared Radiation, Infrared Astronomy, Interstellar Matter, Interstellar Radiation, Radiative Heat Transfer, Supernovae, Graphite, Milky Way Galaxy, Radiant Flux Density, Silicates

Scientific paper

The infrared emission from interstellar grains heated by a supernova in eruption is investigated. The dependence of the emission on various physical parameters, such as the depth of the supernova into the dust plane of the parent galaxy, the inclination of the galaxy to the line-of-sight, are investigated. The possibility of detecting this emission is discussed. The prospects are hopeful as far as cryogenically-cooled instruments in Earth orbit are concerned.

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