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The accretion flow to the intermittent accreting ms pulsar, HETE J1900.1-2455, as observed by XMM-Newton and RXTE
A. Papitto, A. D'Aì, T. Di Salvo +6
We present a study of the accretion flow to the intermittent accreting millisecond pulsar, HETE J1900.1-2455, based on observations performed simultaneously by XMM-Newton and RXTE.…
Observations of Supergiant Fast X-ray Transients with LOFT
E. Bozzo, P. Romano, C. Ferrigno +2
Supergiant Fast X-ray transients are a subclass of high mass X-ray binaries displaying a peculiar and still poorly understood extreme variability in the X-ray domain. These sources…
Investigating Supergiant Fast X-ray Transients with LOFT
P. Romano, E. Bozzo, P. Esposito +2
Supergiant Fast X-ray Transients (SFXT) are a class of High-Mass X-ray Binaries whose optical counterparts are O or B supergiant stars, and whose X-ray outbursts are ~ 4 orders of…
Spectral and timing properties of the accreting X-ray millisecond pulsar IGR J17498-2921
M. Falanga, L. Kuiper, J. Poutanen +5
We analyze the spectral and timing properties of IGR J17498-2921 and the characteristics of X-ray bursts to constrain the physical processes responsible for the X-ray production in…
IGRJ18179-1621: An obscured X-ray pulsar discovered by INTEGRAL
E. Bozzo, C. Ferrigno, M. Tuerler +2
We report on all the INTEGRAL and Swift data collected during the first outburst observed from IGRJ18179-1621. The broad-band spectral analysis showed that the X-ray emission from…
XMM-Newton observations of four high mass X-ray binaries and IGR J17348-2045
E. Bozzo, L. Pavan, C. Ferrigno +5
We present the results of the XMM-Newton observations of five hard X-ray emitters: IGR J08262-3736, IGR J17354-3255, IGR J16328-4726, SAX J1818.6-1703, and IGR J17348-2045. The fir…