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