Abstract
IC 443 is, together with the Cygnus Loop, the best known old supernova remnant. A 21-cm continuum map has been obtained by Duin et al. (communication in this volume), where also references to earlier radio work can be found. IC 443 is very likely associated with an X-ray source (see the communication by Gorenstein in this volume). A pulsar is also probably associated with the remnant (Davies et al.,1972)
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© 1974 D. Reidel Publishing Company, Dordrecht-Holland
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D’odorico, S. (1974). Physical Conditions in the Filaments of SNR from Their Optical Spectra: IC 443. In: Cosmovici, C.B. (eds) Supernovae and Supernova Remnants. Astrophysics and Space Science Library, vol 45. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-2166-1_31
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DOI: https://doi.org/10.1007/978-94-010-2166-1_31
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