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The Swift view of Supergiant Fast X-ray Transients

We report here on the recent results of a monitoring campaign we have been carrying out with Swift/XRT on a sample of four Supergiant Fast X-ray Transients. The main goal of this large programme (with a net Swift/XRT exposure of 540 ks, updated to 2009, August, 31) is to address several main open issues related to this new class of High Mass X-ray Binaries hosting OB supergiant stars as companions. Here we summarize the most important results obtained between October 2007 and August 2009.

preprint2010arXivOpen access
L. SidoliP. RomanoL. DucciA. PaizisS. VercelloneG. CusumanoV. La ParolaV. ManganoD. N. BurrowsJ. A. KenneaH. A. KrimmN. Gehrels
astro-ph.GAastro-ph.HE
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L. SidoliP. RomanoL. DucciA. PaizisS. VercelloneG. CusumanoV. La ParolaV. ManganoD. N. BurrowsJ. A. KenneaH. A. KrimmN. Gehrels

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