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Long-term spectral and timing properties of the soft gamma-ray repeater SGR 1833−0832 and detection of extended X-ray emission around the radio pulsar PSR B1830−08: Observations of SGR 1833−0832 and PSR B1830−08

Monthly Notices of the Royal Astronomical Society(2011)

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摘要
SGR 1833−0832 was discovered on 2010 March 19, thanks to the Swift detection of a short hard X-ray burst and follow-up X-ray observations. Since then, it was repeatedly observed with Swift, Rossi X-ray Timing Explorer and XMM–Newton. Using these data, which span about 225 d, we studied the long-term spectral and timing characteristics of SGR 1833−0832. We found evidence for diffuse emission surrou...
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stars: neutron,pulsars: general,X-rays: individual: PSR B1830−08 (J1833−0827),X-rays: individual: SGR 1833−0832
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