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Gamma Ray Observations from the Crab Nebula and NP-0532

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Supernovae and Supernova Remnants

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 45))

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Abstract

The gamma-ray emission from the Crab Nebula and NP-0532 has been investigated in a series of balloon flights of a multiplate Spark Chamber triggered by a Čerenkov detector-scintillator coincidence system (Parlier et al., 1973; Leray et al., 1972; Vasseur et al., 1971), having a gamma-ray energy threshold for detection at 20 MeV. Figure 1 shows a schematic view of the gamma-ray telescope; Figure 2 the view of the telescope without its thermal protection.

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© 1974 D. Reidel Publishing Company, Dordrecht-Holland

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Parlier, B. et al. (1974). Gamma Ray Observations from the Crab Nebula and NP-0532. 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_30

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  • DOI: https://doi.org/10.1007/978-94-010-2166-1_30

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-2168-5

  • Online ISBN: 978-94-010-2166-1

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