Published March 8, 1965
| Published
Journal Article
Open
Neutron Stars
- Creators
- Bahcall, John N.
-
Wolf, Richard A.
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.Attached Files
Published - BAHprl65a.pdf
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Additional details
- Eprint ID
- 33207
- Resolver ID
- CaltechAUTHORS:20120815-111016825
- Nonr-220(47)
- Office of Naval Research (ONR)
- NGR-05-002-028
- NASA
- NSF Graduate Research Fellowship
- Created
-
2012-08-15Created from EPrint's datestamp field
- Updated
-
2021-11-09Created from EPrint's last_modified field