Bahcall, John N. and Wolf , Richard A. (1965) Neutron Stars. Physical Review Letters, 14 (10). pp. 343-346. ISSN 0031-9007 http://resolver.caltech.edu/CaltechAUTHORS:20120815-111016825
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Several authors have suggested that the recently discovered extraterrestrial sources of x rays may be hot neutron stars. The plausibility of this suggestion, and in fact the likelihood that astronomers will ever be able to observe neutron stars by their x-ray emission, depend critically upon the cooling times of the hot stars.
|Additional Information:||© 1965 American Physical Society. Received 11 January 1965; published in the issue dated 8 March 1965. Work supported in part by the Office of Naval Research [Contract No. Nonr-220(47)] and the National Aeronautics and Space Administration (Contract No. NGR-05-002-028). National Science Foundation Predoctoral Fellow.|
|Official Citation:||Neutron Stars John N. Bahcall and Richard A. Wolf pp. 343-346|
|Usage Policy:||No commercial reproduction, distribution, display or performance rights in this work are provided.|
|Deposited By:||Ruth Sustaita|
|Deposited On:||15 Aug 2012 18:32|
|Last Modified:||26 Dec 2012 15:59|
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