Supergiant Fast X-ray Transients in outburst: new Swift observations of XTE J1739−302, IGR J17544−2619 and IGR J08408−4503

We report on new X-ray outbursts observed with Swift from three Supergiant Fast X-ray Transients (SFXTs): XTE J1739?302, IGR J17544?2619 and IGR J08408?4503. XTE J1739?302 underwent a new outburst on 2008 August 13, IGR J17544?2619 on 2008 September 4 and IGR J08408?4503 on 2008 September 21. While the XTE J1739?302 and IGR J08408?4503 bright emission triggered the Swift /Burst Alert Telescope, IGR J17544?2619 did not, thus we could perform a spectral investigation only of the spectrum below 10 keV. The broad-band spectra from XTE J1739?302 and IGR J08408?4503 were compatible with the X-ray spectral shape displayed during the previous flares. A variable absorbing column density during the flare was observed in XTE J1739?302 for the first time. The broad-band spectrum of IGR J08408?4503 requires the presence of two distinct photon populations, a cold one (～0.3 keV) most likely from a thermal halo around the neutron star and a hotter one (1.4–1.8 keV) from the accreting column. The outburst from XTE J1739?302 could be monitored with a very good sampling, thus revealing a shape which can be explained with a second wind component in this SFXT, in analogy to what we have suggested in the periodic SFXT IGR J11215?5952. The outburst recurrence time-scale in IGR J17544?2619 during our monitoring campaign with Swift suggests a long orbital period of ～150 d (in a highly eccentric orbit), compatible with what previously observed with INTEGRAL .