XMM-Newton observation of the millisecond x-ray pulsar XTE J1751-305 in outburst

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Actively Accreting And Transient Binaries

Scientific paper

XMM-Newton observed XTE J1751-305 for about 35 ksec just 3 days after its discovery. No convincing emission or absorption features are detected in the PN and RGS spectra. The broad band spectrum cannot be fitted with a simple absorbed power-law model, but a blackbody component is also required. The results of the pulse-phase spectroscopy will also be discussed.

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