Magnetospheric Scattering and Emission in Millisecond Pulsars
classification
🌌 astro-ph
keywords
magnetosphericcomponentsemissionmillisecondmodelscatteringaffectedapproximate
read the original 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.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.