268 citations · 4.4k across the 75 of their papers we have counts for
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astro-ph2003★ 64 cited
Spherically symmetric relativistic MHD simulations of pulsar wind nebulae in supernova remnants
N. Bucciantini, J. M. Blondin, L. Del Zanna +1
Pulsars, formed during supernova explosions, are known to be sources of relativistic magnetized winds whose interaction with the expanding supernova remnants (SNRs) gives rise to a…
astro-ph2003★ 93 cited
Signatures of high energy protons in pulsar winds
E. Amato, D. Guetta, P. Blasi
The resonant cyclotron absorption model is very successful in describing particle acceleration in plerions. A sensible prediction of this model is the presence of a substantial amo…