Published March 1990
| Published
Journal Article
Open
A New Class of Pulsars
- Creators
- Backer, Donald C.
-
Kulkarni, Shrinivas R.
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.
Additional Information
© 1990 American Institute of Physics.Attached Files
Published - 1.881227.pdf
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1.881227.pdf
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Additional details
- Eprint ID
- 65661
- Resolver ID
- CaltechAUTHORS:20160324-120454363
- Created
-
2016-03-24Created from EPrint's datestamp field
- Updated
-
2022-10-04Created from EPrint's last_modified field
- Caltech groups
- Division of Geological and Planetary Sciences