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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/2454

Title: The pulsar magnetic window
Authors: Shukre, C.S.
Radhakrishnan, V.
Issue Date: 1981
Publisher: Reidel
Citation: IAU Symposium, 1981, Vol.95, p103
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.
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.
URI: http://hdl.handle.net/2289/2454
Alternative Location: http://adsabs.harvard.edu/cgi-bin/bib_query?1981IAUS...95..103S
Copyright: 1981 Reidel
Appears in Collections:Research Papers (A&A)

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