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- W1972165071 abstract "We report on the results of an EPIC XMM-Newton observation of the faint source SAX J1748.2-2808 and the surrounding field. This source was discovered during the BeppoSAX Galactic center survey performed in 1997–1998. A spatial analysis resulted in the detection of 31 sources within the EPIC field of view. SAX J1748.2-2808 is clearly resolved into 2 sources in EPIC images with the brighter contributing almost 80% of the 2–10 keV flux. Spectral fits to this main source are consistent with an absorbed power-law with a photon index of and absorption equivalent to cm-2 together with an iron line at keV with an equivalent width of eV. The significantly better statistics of the XMM-Newton observation, compared with BeppoSAX, allows to exclude a thermal nature for the X-ray emission. A comparison with other observations of SAXJ1748.2-2808 does not reveal any evidence for spectral or intensity long-term variability. Based on these properties we propose that the source is a low-luminosity high-mass X-ray binary located in the Galactic center region." @default.
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- W1972165071 date "2006-08-23" @default.
- W1972165071 modified "2023-10-18" @default.
- W1972165071 title "Unveiling the nature of the highly absorbed X-ray source SAX J1748.2-2808 with XMM-Newton" @default.
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- W1972165071 doi "https://doi.org/10.1051/0004-6361:20065418" @default.
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