Soft X-rays from IC443

Details Soft X-rays from IC443 Soft X-rays from IC443

Feb 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apl....17...15s&link_type=abstract

Astrophysical Letters, vol. 17, no. 1, 1976, p. 15-17.

Computer Science

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Astronomical Models, Crab Nebula, Supernova Remnants, X Ray Sources, Proportional Counters, Radiation Measurement, Rocket Sounding, Rocket-Borne Instruments, Shock Heating, Sky Surveys (Astronomy), Thermal Emission

Scientific paper

Results are reported for a rocket-borne soft X-ray sky survey which scanned the region including the supernova remnant IC 443 and the Crab Nebula using large-area proportional counters. X-ray emission from IC 443 was detected in the energy range from 0.6 to 1.0 keV. Assuming that shock-heated gas is responsible for this X-ray emission, suggestions are made for obtaining agreement between a thermal emission model and the observations. The possibility is considered that two thermal components may be present in IC 443.

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