Magnetospheric Scattering and Emission in Millisecond Pulsars

Preprint

28 April 2000

preprint
Published by arXiv in arXiv

https://doi.org/10.48550/arXiv.astro-ph/0004407

Abstract

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.

Keywords

MAGNETOSPHERIC SCATTERING
MILLISECOND PULSAR
CURVED SPACE
PROPAGATION
SCATTERING
EMISSION
PULSARS
PHOTON

All Related Versions

Version 1, 2000-04-28, ArXiv
Published version: The Astrophysical Journal, 550 (1), 392.

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