X-ray sources in globular clusters

Details X-ray sources in globular clusters X-ray sources in globular clusters

Dec 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003chjas...3..225v&link_type=abstract

Chinese Journal of Astronomy & Astrophysics, Vol. 3, Supplement, p. 225-234

Astronomy and Astrophysics

Astrophysics

1

Stars: X-Ray Sources, Globular Clusters

Scientific paper

The study of X-ray sources in globular clusters is in very rapid progress, thanks to the combined observations of Chandra and XMM X-ray observatories, and the Hubble Space Telescope. In addition to the low-mass X-ray binaries known since the early 1970s, quiescent X-ray binaries, cataclysmic variables, radio pulsars, and magnetically active binaries can now be identified and studied in X-rays and optical. This improves our knowledge of the population of binaries in globular clusters.

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