Magnetospheric Scattering and Emission in Millisecond Pulsars

Astronomy and Astrophysics – Astrophysics

Scientific paper

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submitted to ApJ

Scientific paper

10.1086/319706

We model the formation of magnetospheric components of millisecond pulsar
light curves, deriving an approximate model for the curved space, `swept-back'
dipole field and following photon emission, propagation, and scattering.
Magnetospheric pulse components are strongly affected by rapid rotation and
Schwarzschild effects.

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