Isolated Neutron Stars
V. M. Kaspi, M. S. E. Roberts (McGill), A. K. Harding (GSFC)
TL;DR
This review paper discusses the X-ray emission mechanisms of various isolated neutron stars, focusing on rotation-powered pulsars, including their magnetospheric, thermal emissions, and associated pulsar wind nebulae.
Contribution
It provides a comprehensive overview of the current understanding of X-ray emissions from isolated neutron stars, emphasizing recent observational and theoretical developments.
Findings
Detailed characterization of magnetospheric and thermal X-ray emissions.
Insights into pulsar wind nebulae structures and dynamics.
Summary of observational data across different neutron star types.
Abstract
This is a review of X-ray emission from all types of isolated neutron stars, with an emphasis on rotation-powered pulsars. Topics include magnetospheric and thermal emission, as well as pulsar wind nebulae.
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Geophysics and Sensor Technology · Geophysics and Gravity Measurements