INTEGRAL observations of IGRJ11215-5952: the first Supergiant Fast X-ray Transient displaying periodic outbursts
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The hard X-ray source IGRJ11215-5952, discovered with INTEGRAL during a brief outburst in 2005, has been proposed as a new member of the class of Supergiant Fast X-ray Transients. Analysing archival INTEGRAL observations of the source field,we have discovered two previously unnoticed outbursts (in July 2003 and in May 2004),spaced by intervals of ~330 days, suggesting a possible orbital period.The 5-100keV spectrum is well described by a cut-off power law, with a photon index of 0.5, and a cut-off energy 15-20keV, typical of High Mass X-ray Binaries containing a neutron star. The luminosity is ~3E36erg/s assuming 6.2kpc, the distance of the likely optical counterpart, the blue supergiant HD306414.A fourth outburst was discovered in 2006 with XTE/PCA, 329 days after the third one, confirming the periodic nature of the source outbursts.Follow-up observations with Swift/XRT refined the source position and confirmed the association with HD306414.The 5-100keV spectrum, the recurrent nature of the outbursts, the blue supergiant companion star HD 306414, support the hypothesis that IGRJ11215-5952 is a Supergiant Fast X-ray Transient, and it is the first object of this class of High Mass X-ray Binaries displaying periodic outbursts.
To be published in the proceedings of the conference "The Multicoloured Landscape of Compact Objects and their Explosive Origins", eds.L.Burderi et al., held in Cefalu', Sicily (Italy), June 11-24, 2006. Submitted
To be published in the proceedings of the conference "The Multicoloured Landscape of Compact Objects and their Explosive Origins", eds.L.Burderi et al., held in Cefalu', Sicily (Italy), June 11-24, 2006. Submitted