An X-ray view of millisecond pulsars

Details An X-ray view of millisecond pulsars An X-ray view of millisecond pulsars

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..599...13b&link_type=abstract

X-RAY ASTRONOMY: Stellar Endpoints,AGN, and the Diffuse X-ray Background. Edited by Nicholas E. White, Giuseppe Malaguti, and G

Astronomy and Astrophysics

Astronomy

5

X-Ray Sources, X-Ray Bursts, Pulsars, Observatories And Site Testing

Scientific paper

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. .

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