Published March 8, 1965 | Version Published
Journal Article Open

Neutron Stars

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.

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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Identifiers

Eprint ID
33207
Resolver ID
CaltechAUTHORS:20120815-111016825

Funding

Office of Naval Research (ONR)
Nonr-220(47)
NASA
NGR-05-002-028
NSF Graduate Research Fellowship

Dates

Created
2012-08-15
Created from EPrint's datestamp field
Updated
2021-11-09
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