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Neutron star masses from hydrodynamical effects in obscured sgHMXBs
A. Manousakis, R. Walter, J. M. Blondin
A population of obscured supergiant High Mass X-ray Binaries (sgHMXBs) has been discovered by INTEGRAL. X-ray wind tomography of IGR J17252-3616 inferred a slow wind velocity to ac…
A stacking method to study the gamma-ray emission of source samples based on the co-adding of Fermi LAT count maps
B. Huber, C. Farnier, A. Manalaysay +2
We present a stacking method that makes use of co-added maps of gamma-ray counts produced from data taken with the Fermi Large Area Telescope. Sources with low integrated gamma-ray…
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…
XMM-Newton Finds That SAX J1750.8-2900 May Harbor the Hottest, Most Luminous Known Neutron Star
Alexander W. Lowell, John A. Tomsick, Craig O. Heinke +6
We have performed the first sensitive X-ray observation of the low-mass X-ray binary SAX J1750.8-2900 in quiescence with XMM-Newton. The spectrum was fit to both a classical black…