Cooling and evolution of adiabatic blast waves in a dusty medium

Details Cooling and evolution of adiabatic blast waves in a dusty medium Cooling and evolution of adiabatic blast waves in a dusty medium

Jul 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981apj...247..614d&link_type=abstract

Astrophysical Journal, Part 1, vol. 247, July 15, 1981, p. 614-627.

Astronomy and Astrophysics

Astrophysics

27

Cosmic Dust, Detonation Waves, Infrared Radiation, Interstellar Matter, Radiant Cooling, Supernova Remnants, Adiabatic Conditions, Collisional Plasmas, Energy Dissipation, Granular Materials, Luminous Intensity, Nebulae, Particle Collisions, Plasma Heating

Scientific paper

Detailed numerical calculations are presented of the cooling and destruction of collisionally heated interstellar dust grains that are swept up by adiabatic supernova blast waves. The infrared luminosity that is emitted from the interior of the supernova cavity is calculated, and the effect of the energy loss on the evolution of the remnant is studied. Recent observations of several young supernova remnants are briefly discussed.

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