Kulkarni, S. R. and Thompson, Christopher (1998) Neutron stars: A star powered by magnetism. Nature, 393 (6682). pp. 215-216. ISSN 0028-0836. https://resolver.caltech.edu/CaltechAUTHORS:20150610-105911648
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Abstract
Ever since their discovery three decades ago, neutron stars have fascinated astronomers. They have extreme properties in almost all respects: they are the densest objects in the Universe, the most rapidly rotating, and the best astronomical laboratory for condensed-matter physics. To this, Kouveliotou et al. (page 235 of this issue) add direct evidence of magnetic fields strong enough to perturb the very structure of the vacuum.
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| Additional Information: | © 1998 Macmillan Publishers Ltd. | ||||||||||||
| Issue or Number: | 6682 | ||||||||||||
| Record Number: | CaltechAUTHORS:20150610-105911648 | ||||||||||||
| Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20150610-105911648 | ||||||||||||
| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | ||||||||||||
| ID Code: | 58154 | ||||||||||||
| Collection: | CaltechAUTHORS | ||||||||||||
| Deposited By: | Tony Diaz | ||||||||||||
| Deposited On: | 10 Jun 2015 18:31 | ||||||||||||
| Last Modified: | 03 Oct 2019 08:33 |
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