The pulsar magnetic window

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DC Field	Value	Language
dc.contributor.author	Shukre, C.S.	-
dc.contributor.author	Radhakrishnan, V.	-
dc.date.accessioned	2007-05-25T09:24:50Z	-
dc.date.available	2007-05-25T09:24:50Z	-
dc.date.issued	1981	-
dc.identifier.citation	IAU Symposium, 1981, Vol.95, p103	en
dc.identifier.uri	http://hdl.handle.net/2289/2454	-
dc.description	Open Access. Pulsars: 13 years of research on neutron stars; Proceedings of the Symposium, Bonn, West Germany, August 26-29, 1980. (A82-32926 15-90) Dordrecht, D. Reidel Publishing Co.	en
dc.description.abstract	Triggering of the spark discharges in the Ruderman and Sutherland (1975) model by background gamma rays is shown to be effective only within a narrow range of neutron star magnetic fields centered on 2.5 x 10 to the 12th gauss. This calculated range of field strengths is in good agreement with 'observed' values, suggesting that (1) such triggering is operative, and (2) that neutron stars with much stronger fields do not function as pulsars.	en
dc.format.extent	214900 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Reidel	en
dc.relation.uri	http://adsabs.harvard.edu/cgi-bin/bib_query?1981IAUS...95..103S	en
dc.rights	1981 Reidel	en
dc.title	The pulsar magnetic window	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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