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Stellar Accretion and X-ray Emission

Nature volume 215, pages 464–466 (1967)Cite this article

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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Author information

Authors and Affiliations

  1. Belfer Graduate School of Science, Yeshiva University, New York

    A. G. W. CAMERON

  2. Institute for Space Studies, Goddard Space Flight Center, NASA, New York

    A. G. W. CAMERON

  3. Department of Physics, Columbia University, New York

    M. MOCK

  4. Institute for Space Studies, Goddard Space Flight Center, NASA, New York

    M. MOCK

Authors
  1. A. G. W. CAMERON
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  2. M. MOCK
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CAMERON, A., MOCK, M. Stellar Accretion and X-ray Emission. Nature 215, 464–466 (1967). https://doi.org/10.1038/215464a0

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