An analytical solution for the infrared emission from interstellar grains heated by supernovae

Details An analytical solution for the infrared emission from interstellar grains heated by supernovae An analytical solution for the infrared emission from interstellar grains heated by supernovae

Nov 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...169..380p&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 169, no. 1-2, Nov. 1986, p. 380-382.

Astronomy and Astrophysics

Astrophysics

Infrared Spectra, Interstellar Matter, Radiative Heat Transfer, Supernovae, Astronomical Models, Mass Flow, Supernova Remnants

Scientific paper

An analytical solution is described for the heating of interstellar grains by an erupting supernova. Two cases are considered and the analytical solutions obtained are compared to the corresponding numerical solutions. Good agreement is found to exist between analytical and numerical solutions. It is concluded that such an analytical solution may be used to give an order of magnitude estimate of the infrared fluxes obtained due to the heating of interstellar grains by erupting supernovae.

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