On the Geometry of the X-Ray Emission from Pulsars. I. Model Formulation and Tests
Author:
Funder
Astrophysics Science Division
Publisher
IOP Publishing
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/1538-3873/129/i=982/a=124201/pdf
Reference47 articles.
1. An ultraluminous X-ray source powered by an accreting neutron star
2. The Limiting Luminosity of Accreting Neutron Stars With Magnetic Fields
3. Spectral Formation in X‐Ray Pulsars: Bulk Comptonization in the Accretion Shock
4. Dynamical Structure of Radiation‐dominated Pulsar Accretion Shocks
5. Gravitational Bending of Light Near Compact Objects
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