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Is Crab nebula a disrupted helium star? (1979)

KOCHHAR, R. K.

[s.l.] : Nature Publishing Group

Nature 277 (1979), S. 116-116

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ISSN: 1476-4687

Source: Nature Archives 1869 - 2009

Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics

Notes: [Auszug] Arnett has pointed out that the overabundance of helium with respect to hydrogen in the Crab filaments2 is compatible with a presupernova helium core of mass 4 M0 (rf. 3) which corresponds to a main sequence mass of 12 M (rf. 4). Chevalier5, on examining old Chinese records, present day nebula and ...

Type of Medium: Electronic Resource

URL: http://dx.doi.org/10.1038/277116a0

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