Publication Abstracts

Cameron and Mock 1967

Cameron, A.G.W., and M. Mock, 1967: Stellar accretion and X-ray emission. Nature, 215, 464-466, doi:10.1038/215464a0.

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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BibTeX Citation

  author={Cameron, A. G. W. and Mock, M.},
  title={Stellar accretion and X-ray emission},

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RIS Citation

ID  - ca07810a
AU  - Cameron, A. G. W.
AU  - Mock, M.
PY  - 1967
TI  - Stellar accretion and X-ray emission
JA  - Nature
JO  - Nature
VL  - 215
SP  - 464
EP  - 466
DO  - 10.1038/215464a0
ER  -

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