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Causal Relationship between Drifting Subpulse Parameters and Some Pulsar Quantities

Published online by Cambridge University Press:  27 September 2017

Natasha Shapirovskaya
Natasha Shapirovskaya*
Affiliation:
Astro Space Center, P. N. Lebedev Physical Institute

Abstract

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Correlation analysis of subpulse spacing P2, subpulse bands P3, subpulse drift rate with some quantities such as pulsar period P, profile width We, characteristic age r and others indicates some new casual dependencies not previously confirmed. Relations obtained in this paper possibly point out that interaction between pulsar radio emission and the interstellar environment may exert some influence on the drift appearance.

Type
Part VII Polar cap phenomena
Information
International Astronomical Union Colloquium , Volume 128: Magnetospheric structure and emission mechanisms of radio pulsars , 1992 , pp. 293 - 295
Copyright
Copyright © United States Naval Observatory 1992