Model for the microstructure emission of pulsars
Open Access
- 1 July 1977
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 179 (3) , 311-315
- https://doi.org/10.1093/mnras/179.3.311
Abstract
We use the recent observations of Rickett, Hankins & Cordes to construct a qualitative model of the emitting region near pulsars. Their data can be reconciled with the view that dense regions, themselves containing many coherent radiating filaments, extend for long distances along the dipolar field lines.Keywords
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