Three-dimensional analytical description of magnetized winds from oblique pulsars
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/457/3/3384/7999855/stv2869.pdf
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1. Pulsed high-energyγ-rays from thermal populations in the current sheets of pulsar winds
2. An ultraluminous X-ray source powered by an accreting neutron star
3. Collisional mechanism for gamma-ray burst emission
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5. Dissipation, energy transfer, and spin-down luminosity in 2.5D PIC simulations of the pulsar magnetosphere
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