Time-dependent 3D magnetohydrodynamic pulsar magnetospheres: oblique rotators
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnrasl/article-pdf/435/1/L1/3823710/slt076.pdf
Reference44 articles.
1. Pulsed high-energyγ-rays from thermal populations in the current sheets of pulsar winds
2. UNCERTAINTIES OF MODELING GAMMA-RAY PULSAR LIGHT CURVES USING VACUUM DIPOLE MAGNETIC FIELD
3. MODELING OF GAMMA-RAY PULSAR LIGHT CURVES USING THE FORCE-FREE MAGNETIC FIELD
4. Relativistic magnetohydrodynamics winds from rotating neutron stars
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