Backer, Donald C. and Kulkarni, Shrinivas R. (1990) A New Class of Pulsars. Physics Today, 43 (3). pp. 26-35. ISSN 00319228. doi:10.1063/1.881227. https://resolver.caltech.edu/CaltechAUTHORS:20160324-120454363
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Abstract
In 1939, seven years after the discovery of the neutron, nuclear physicists constructed the first models of a "neutron star." Stable results were found with masses comparable to the Sun's radii of about 10 km. Binary pulsars, pulsars with millisecond periods and pulsars in globular clusters are distinguished by their evolutionary histories, and are providing tools for fundamental tests of physics.
| Item Type: | Article | |||||||||
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| Additional Information: | © 1990 American Institute of Physics. | |||||||||
| Issue or Number: | 3 | |||||||||
| DOI: | 10.1063/1.881227 | |||||||||
| Record Number: | CaltechAUTHORS:20160324-120454363 | |||||||||
| Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20160324-120454363 | |||||||||
| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | |||||||||
| ID Code: | 65661 | |||||||||
| Collection: | CaltechAUTHORS | |||||||||
| Deposited By: | Joy Painter | |||||||||
| Deposited On: | 24 Mar 2016 19:37 | |||||||||
| Last Modified: | 10 Nov 2021 23:48 |
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