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Discovery of an X-ray source coincident with the soft γ-ray repeater 0525 - 66

Rothschild, R. E. and Kulkarni, S. R. and Lingenfelter, R. E. (1994) Discovery of an X-ray source coincident with the soft γ-ray repeater 0525 - 66. Nature, 368 (6470). pp. 432-434. ISSN 0028-0836. https://resolver.caltech.edu/CaltechAUTHORS:20150609-144301671

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Abstract

ALTHOUGH γ-ray bursters (GRBs) have been known for more than 20 years, no source has ever been identified in its quiescent state, which might provide clues to its nature. On the other hand, two of the three known soft γ-ray repeaters (SGRs), which emit intermittent bursts of soft γ-rays, seem to be associated with supernova remnants and the recent identification of X-rays from one of these, SGR1806 – 20, supports the suggestion that a pulsar inside the remnant is the source of the γ-rays. Here we report X-ray observations of SGR0525 – 66, which has been associated previously with the supernova remnant N49 (ref. 1). We identify point-like emission from a source coincident with SGR0525 – 66, which suggests that it too is a pulsar. The pulsar seems to be only about 5,000 years old and has a high transverse velocity of about 1,200 km s^(−1), and we predict that the plerion (the region of radio synchrotron emission surrounding the pulsar) will be between 0.1 and 0.3 arcsec across. A high birth velocity has been estimated for the pulsar associated with SGR1806 – 20 also, and this characteristic may be related to the reason why only a very few pulsars become SGRs.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1038/368432a0DOIArticle
http://www.nature.com/nature/journal/v368/n6470/abs/368432a0.htmlPublisherArticle
ORCID:
AuthorORCID
Kulkarni, S. R.0000-0001-5390-8563
Additional Information:© 1994 Nature Publishing Group. Received 10 November 1993; accepted 10 February 1994. We thank R. Petre, M. Corcoran, and the Rosat Data Center duty scientists for assisting with the understanding of the data and its analysis, and O. Vancura for providing the optical images of N49. R.E.R. and R.E.L. are supported by NASA. S.R.K. is supported by US NSF, NASA and the Packard foundation.
Funders:
Funding AgencyGrant Number
NASAUNSPECIFIED
NSFUNSPECIFIED
David and Lucile Packard FoundationUNSPECIFIED
Issue or Number:6470
Record Number:CaltechAUTHORS:20150609-144301671
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20150609-144301671
Official Citation:Discovery of an X-ray source coincident with the soft γ-ray repeater 0525 – 66 432 R. E. Rothschild, S. R. Kulkarni & R. E. Lingenfelter doi:10.1038/368432a0
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:58136
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:10 Jun 2015 15:31
Last Modified:03 Oct 2019 08:32

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