Abstract:INTEGRAL allowed the discovery of several new SuperGiant X-ray Binaries of which very few were known before its launch. Among them, INTEGRAL has unveiled a new sub-class: galactic X-ray sources with a supergiant companion and displaying a transient behaviour, namely Supergiant Fast X-ray Transient. Most of the time in quiescence with a luminosity of 10 33 erg s −1 (if not totally absent), these sources display rare episodes of short (few ks) and bright (up to ∼ 10 36 erg s −1 as in other SGXB) flares. Several … Show more
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