Infrared radiation from evaporating clouds

Details Infrared radiation from evaporating clouds Infrared radiation from evaporating clouds

Jun 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981apj...246..430d&link_type=abstract

Astrophysical Journal, Part 1, vol. 246, June 1, 1981, p. 430-433.

Astronomy and Astrophysics

Astrophysics

9

Cosmic Dust, Evaporation, Infrared Radiation, Interstellar Gas, Nebulae, Supernova Remnants, Gas Density, Gas Flow, Gas Temperature, Stellar Evolution

Scientific paper

It is shown that dusty clouds that evaporate into a hot ambient medium may, under certain astrophysical conditions, be important sources of infrared radiation. The infrared radiation is emitted by collisionally heated dust grains that are present in the evaporate flow. The resulting enhancement in the cooling rate of the intercloud gas may have an important effect on the evolution of young supernova remnants.

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