Chandra and XMM-Newton Observations of Millisecond Pulsars in Globular Clusters and the Field of the Galaxy

Details Chandra and XMM-Newton Observations of Millisecond Pulsars in Globular Clusters and the Field of the Galaxy Chandra and XMM-Newton Observations of Millisecond Pulsars in Globular Clusters and the Field of the Galaxy

Feb 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010head...11.2304b&link_type=abstract

American Astronomical Society, HEAD meeting #11, #23.04; Bulletin of the American Astronomical Society, Vol. 41, p.694

Astronomy and Astrophysics

Astronomy

Scientific paper

I will present the results of recent deep Chandra and XMM-Newton observations of rotation-powered ("recycled") millisecond pulsars
both in the field of the Galaxy and in the globular clusters NGC 6397 and M28. In addition to elucidating the general X-ray properties of the Galactic millisecond pulsar population, these studies have demonstrated that millisecond pulsars can potentially serve as precision probes of neutron star structure as well as internal globular cluster dynamics, close binary evolution, relativistic pulsar winds, and collisionless shock.

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