Finding fast spinning neutron stars using XMM-Newton

Authors
Publication date 2008
Host editors
  • R. Wijnands
  • D. Altamirano
  • P. Soleri
  • N. Degenaar
  • N. Rea
  • P. Casella
  • A. Patruno
  • M. Linares
Book title A Decade of Accreting Millisecond X-ray Pulsars
Book subtitle proceedings of the international workshop, Amsterdam, the Netherlands, 14-18 April 2008
ISBN
  • 9780735405998
Series AIP Conference Proceedings
Event A Decade of Accreting Millisecond X-ray Pulsars, Amsterdam, the Netherlands
Pages (from-to) 231-234
Publisher Melville, NY: American Institute of Physics
Organisations
  • Faculty of Science (FNWI) - Anton Pannekoek Institute for Astronomy (API)
Abstract
The discovery of millisecond X-ray pulsations in neutron-star low-mass X-ray binaries has until now only been done with the Rossi X-ray Timing Explorer. However, XMM-Newton has also pointed at some of these systems during an outburst and shown that it can clearly detect the pulsations as well. In fact, XMM-Newton detects the pulsations with high enough significance to have discovered them, had they still been unknown. Thus, XMM-Newton can also be used to search for pulsations. Moreover, for the faintest systems XMM-Newton is even more sensitive to detect pulsations than RXTE due to the significantly less background count rate for XMM-Newton.
Document type Conference contribution
Language English
Published at https://doi.org/10.1063/1.3031198
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