Finding fast spinning neutron stars using XMM-Newton
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| Publication date | 2008 |
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| 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 |
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| 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 |
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| 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.
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| Document type | Conference contribution |
| Language | English |
| Published at | https://doi.org/10.1063/1.3031198 |
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