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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Abstract
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.
| Item Type: | Article | ||||||||
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| 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. | ||||||||
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| Record Number: | CaltechAUTHORS:20120815-111016825 | ||||||||
| Persistent URL: | http://resolver.caltech.edu/CaltechAUTHORS:20120815-111016825 | ||||||||
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| 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. | ||||||||
| ID Code: | 33207 | ||||||||
| Collection: | CaltechAUTHORS | ||||||||
| Deposited By: | Ruth Sustaita | ||||||||
| Deposited On: | 15 Aug 2012 18:32 | ||||||||
| Last Modified: | 26 Dec 2012 15:59 |
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