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• W2074133046 abstract "IGR J18483-0311 was discovered with INTEGRAL in 2003 and later classified as a supergiant fast X-ray transient. It was observed in outburst many times, but its quiescent state is still poorly known. Here we present the results of XMM-Newton, Swift, and Chandra observations of IGRJ18483-0311. These data improved the X-ray position of the source, and provided new information on the timing and spectral properties of IGR J18483-0311 in quiescence. We report the detection of pulsations in the quiescent X-ray emission of this source, and give for the first time a measurement of the spin-period derivative of this source. In IGRJ18483-0311 the measured spin-period derivative of -(1.3+-0.3)x10^(-9) s/s likely results from light travel time effects in the binary. We compare the most recent observational results of IGRJ18483-0311 and SAXJ1818.6-1703, the two supergiant fast X-ray transients for which a similar orbital period has been measured." @default.
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• W2074133046 date "2009-10-21" @default.
• W2074133046 modified "2023-10-01" @default.
• W2074133046 title "The supergiant fast X-ray transient IGR J18483−0311 in quiescence:<i>XMM-Newton</i>,<i>Swift</i>and<i>Chandra</i>observations" @default.
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• W2074133046 doi "https://doi.org/10.1111/j.1365-2966.2009.15174.x" @default.
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