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X-Rays From Millisecond Pulsars

  • Werner Becker
Part of the Astrophysics and Space Science Library book series (ASSL, volume 254)

Abstract

The satellite observatories ROSAT, ASCA, RXTE and BeppoSAX have brought important progress in neutron star and pulsar astronomy. With significantly higher sensitivities compared with previous X-ray satellites they allowed for the first time to detect X-ray emission from objects as faint as millisecond (ms) pulsars. In this paper we summarize the current observational status and discuss the empirical constraints on the pulsars’ X-ray emission mechanisms.

Keywords

Neutron Star Millisecond Pulsar Pulse Profile Pulse Component ASCA Data 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer Science+Business Media Dordrecht 2000

Authors and Affiliations

  • Werner Becker
    • 1
  1. 1.Max-Planck-Institut für extraterrestrische PhysikGarchingGermany

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