Emission altitudes in young and old radio pulsars
arXiv:astro-ph/0101429 · doi:10.1046/j.1365-8711.2001.04302.x
Abstract
The paper presents a comparison of emission altitudes in very young and very old radio pulsars. The author confirmes that altitudes at which radio emission at a given frequency is generated depend on pulsar period and on pulsar age, although the latter dependence is quite weak.
7 pages, LaTex, 3 PS figures, accepted for publication in MNRAS
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