Stellar Accretion and X-ray Emission

descriptionPublicationkeyboard_double_arrow_right Article 01 Jul 1967 English Publisher:Springer Science and Business Media LLCJournal:Nature, volume 215, pages 464-466 (issn: 0028-0836, eissn: 1476-4687,

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Authors: A. G. W. CAMERON; M. MOCK;

doi: 10.1038/215464a0

Stellar Accretion and X-ray Emission

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Abstract

Shklovsky has suggested that the Scorpius X-ray source is a binary pair and that the X-radiation arises from the collision of material from a giant star with a neutron star. The theoretical complications of such a model are now found not to match actual measurements and it is suggested that the bremsstrahlung effect occurs between a giant star and a white dwarf.

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