Modelling the bow shock Pulsar Wind Nebulae propagating through a non-uniform ISM
Author:
Affiliation:
1. Space Research Institute, Russian Academy of Sciences, Profsoyuznaya 84/32, Moscow 117997, Russia
2. Department of Astronomy, Cornell University, Ithaca, NY 14853-6801
Funder
National Aeronautics and Space Administration
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/484/2/1475/27583135/stz034.pdf
Reference53 articles.
1. THE THEORY OF PULSAR WIND NEBULAE
2. Electron density power spectrum in the local interstellar medium
3. Theory of pulsar winds
4. Relativistic particle acceleration in plerions
5. The Velocity Distribution of Isolated Radio Pulsars
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