Abstract
Supernova remnants ware the first class of X-ray emitting objects to be positively identified. Indeed they were the only sources of X-ray emission to be predicted as such before the beginning of observational X-ray astronomy in 1962. While the use of X-ray detection systems on sounding rockets lead to a number of advances in the study of remnants, spectacular progress has followed the availability of satellite borne instruments.
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Culhane, J.L. (1977). X-rays from Supernova Remnants. In: Schramm, D.N. (eds) Supernovae. Astrophysics and Space Science Library, vol 66. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-1229-4_4
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DOI: https://doi.org/10.1007/978-94-010-1229-4_4
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