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[Ni II] Emission in Supernova Remnants
Published online by Cambridge University Press: 12 April 2016
Abstract
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Combining new spectrophotometric data on the Orion and Crab Nebulae with detailed calculations, we show that strong [Ni II] λ7378 emission observed in numerous SNR’s may be associated with gas having Ne > 50,000 cm−3.
- Type
- Research Article
- Information
- International Astronomical Union Colloquium , Volume 101: Supernova Remnants and the Interstellar Medium , 1988 , pp. 183 - 186
- Copyright
- Copyright © Cambridge University Press 1988
References
Henry, R.B.C.
1984a, in Stellar Nucleosynthesis, ed. Chiosi, C. and Renzini, A. (Dordrecht: Reidel), p. 43.CrossRefGoogle Scholar