Emission from the sub-millisecond pulsar in SN 1987A

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4349

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DC Field	Value	Language
dc.contributor.author	Sivaram, C	-
dc.contributor.author	de Sabbata, V	-
dc.date.accessioned	2009-02-06T12:01:23Z	-
dc.date.available	2009-02-06T12:01:23Z	-
dc.date.issued	1990	-
dc.identifier.citation	Proceedings of the 21st International Cosmic Ray Conference. Vol. 2, (OG Sessions), pp. 250 - 253	en
dc.identifier.uri	http://hdl.handle.net/2248/4349	-
dc.description.abstract	We consider the production and emission of high energy particles from the sub millisecond pulsar, newly discovered in SN 1987A. We also discuss the emission of very high energy gamma rays and other electromagnetic radiation from the pulsar surface and magnetosphere including possible pleirons and cavities. Constraints are put on some of the current models of particle acceleration in pulsars. The evolution of such pulsars and their contribution to the energy cosmic ray background is studied.	en
dc.language.iso	en	en
dc.publisher	International Cosmic Ray	en
dc.relation.ispartofseries	International Cosmic Ray Conference, Vol. 2	-
dc.relation.uri	http://adsabs.harvard.edu/abs/1990ICRC....2..250S	en
dc.subject	Sub-Millisecond Pulsar	en
dc.subject	Pulsar: SN 1987A	en
dc.title	Emission from the sub-millisecond pulsar in SN 1987A	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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