Abstract
Spectral index variations in supernova remnants are reviewed. In case of S147 the total emission is decomposed into small-scale and large-scale diffuse emission. Both components have different radio spectra. Possible consequences on the nature of the optical filaments in 5147 are indicated.
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© 1988 Springer-Verlag
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Fürst, E., Reich, W. (1988). Spectral index variations in supernova remnants. In: Kundt, W. (eds) Supernova Shells and Their Birth Events. Lecture Notes in Physics, vol 316. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-50435-4_4
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DOI: https://doi.org/10.1007/3-540-50435-4_4
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