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Neutron stars: A star powered by magnetism

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.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1038/30357 DOIArticle
http://www.nature.com/nature/journal/v393/n6682/full/393215a0.htmlPublisherArticle
http://rdcu.be/c4MTPublisherFree ReadCube access
ORCID:
AuthorORCID
Kulkarni, S. R.0000-0001-5390-8563
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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