Confirmation of the supergiant fast X‐ray transient nature of AX J1841.0−0536 from Swift outburst observations

@article{Romano2010ConfirmationOT,
  title={Confirmation of the supergiant fast X‐ray transient nature of AX J1841.0−0536 from Swift outburst observations},
  author={Patrizia Romano and Vanessa Mangano and G Cusumano and Paolo Esposito and P. A. Evans and Jamie A. Kennea and Stefano Vercellone and Valentina La Parola and H A Krimm and David N. Burrows and N. Gehrels INAFIASF-Palermo and INAF-OA Cagliari and University of Leicester and Psu and NasaGsfc and Usra},
  journal={Monthly Notices of the Royal Astronomical Society: Letters},
  year={2010},
  volume={412}
}
  • P. Romano, V. Mangano, +13 authors Usra
  • Published 2010
  • Physics
  • Monthly Notices of the Royal Astronomical Society: Letters
Swift observed an outburst from the supergiant fast X-ray transient (SFXT) AX J1841.0−0536 on 2010 June 5, and followed it with X-ray Telescope (XRT) for 11 d. The X-ray light curve shows an initial flare followed by a decay and subsequent increase, as often seen in other SFXTs, and a dynamical range of ∼1600. Our observations allow us to analyse the simultaneous broad-band (0.3–100 keV) spectrum of this source, for the first time down to 0.3 keV, which can be fitted well with models usually… Expand

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