The pulsar magnetic window
| 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.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.identifier.citation | IAU Symposium, 1981, Vol.95, p103 | en |
| dc.identifier.uri | http://hdl.handle.net/2289/2454 | |
| 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 |