Time evolution of pulsar obliquity angle from 3D simulations of magnetospheres
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/441/3/1879/3868553/stu591.pdf
Reference37 articles.
1. UNCERTAINTIES OF MODELING GAMMA-RAY PULSAR LIGHT CURVES USING VACUUM DIPOLE MAGNETIC FIELD
2. MODELING OF GAMMA-RAY PULSAR LIGHT CURVES USING THE FORCE-FREE MAGNETIC FIELD
3. The influence of nondipolar magnetic field and neutron star precession on braking indices of radiopulsars
4. On the mean profiles of radio pulsars - I. Theory of propagation effects
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