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- W3098984251 abstract "SAX J1711.6-3808 is an X-ray transient in the Galactic bulge that was active from January through May of 2001 and whose maximum 1–200 keV luminosity was measured to be $5times 10^{-9}$ erg cm -2 s -1 which is less than ~25% of the Eddington limit, if placed at a distance equal to that of the galactic center. We study the X-ray data that were taken of this moderately bright transient with instruments on BeppoSAX and RXTE. The spectrum shows two interesting features on top of a Comptonized continuum commonly observed in low-state X-ray binaries: a broad emission feature peaking at 7 keV and extending from 4 to 9 keV, and a soft excess with a color temperature below 1 keV which reveals itself only during one week of data. High time-resolution analysis of 412 ksec worth of data fails to show bursts, coherent or high-frequency quasi-periodic oscillations. Given the dynamic range of the flux measurements, this would be unusual if a neutron star were present. SAX J1711.6-3808 appears likely to contain a black hole. No quiescent optical counterpart could be identified in archival data within the 5´´-radius XMM error circle, but the limits are not very constraining because of heavy extinction ($A_{ V}=16$)." @default.
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- W3098984251 date "2002-07-12" @default.
- W3098984251 modified "2023-09-23" @default.
- W3098984251 title "The nature of the X-ray transient SAX J1711.6-3808" @default.
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- W3098984251 doi "https://doi.org/10.1051/0004-6361:20020762" @default.
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