Search for far-infrared emission from young supernova remnants

Details Search for far-infrared emission from young supernova remnants Search for far-infrared emission from young supernova remnants

Sep 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...240l.157w&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 240, Sept. 15, 1980, p. L157, L158.

Astronomy and Astrophysics

Astrophysics

18

Far Infrared Radiation, Infrared Stars, Radio Emission, Supernova Remnants, Nebulae, Radiant Flux Density, Thermal Emission, X Ray Sources

Scientific paper

A search has been conducted for 80-350 micron emission from the Tycho, Kepler, and Cas A supernova remnants. The bolometric fluxes are less than 5 x 10 to the -11th, 4 x 10 to the -12th, and 9 x 10 to the -12th W/sq m, respectively, for the entire radio shell, corresponding to luminosities less than 25,000, 1100, and 1500 solar luminosities (within 2 standard deviations). The ratio of dust to gas in Cas A is at least 10 times less than the 'normal' ratio.

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