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Neutron Stars

Bahcall, John N. and Wolf, Richard A. (1965) Neutron Stars. Physical Review Letters, 14 (10). pp. 343-346. ISSN 0031-9007. https://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
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1103/PhysRevLett.14.343DOIArticle
ORCID:
AuthorORCID
Wolf, Richard A.0000-0001-5291-4275
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.
Funders:
Funding AgencyGrant Number
Office of Naval Research (ONR)Nonr-220(47)
NASANGR-05-002-028
NSF Graduate Research FellowshipUNSPECIFIED
Issue or Number:10
Record Number:CaltechAUTHORS:20120815-111016825
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20120815-111016825
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:23 Nov 2020 19:44

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