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• W4300882600 abstract "We present the results of the first four (quasi-)simultaneous radio (ATCA), X-ray (Swift, RXTE), and γ-ray (INTEGRAL) observations of the black hole candidate IGR J17091−3624, performed in February and March 2011. The X-ray analysis shows that the source was in the hard state, and then it transited to a soft intermediate state. We study the correlated radio/X-ray behaviour of this source for the first time. The radio counterpart to IGR J17091−3624 was detected during all four observations with the ATCA. In the hard state, the radio spectrum is typical of optically thick synchrotron emission from a self-absorbed compact jet. In the soft intermediate state, the detection of optically thin synchrotron emission is probably due to a discrete ejection event associated with the state transition. The position of IGR J17091−3624 in the radio versus X-ray luminosity diagram (aka fundamental plane) is compatible with that of the other black hole sources for distances greater than 11 kpc. IGR J17091−3624 also appears as a new member of the few sources that show a strong quenching of radio emission after the state transition. Using the estimated luminosity at the spectral transition from the hard state, and for a typical mass of 10 M⊙, we estimate a distance to the source between ~11 and ~17 kpc, compatible with the radio behaviour of the source." @default.
• W4300882600 created "2022-10-04" @default.
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• W4300882600 date "2011-08-22" @default.
• W4300882600 modified "2023-10-09" @default.
• W4300882600 title "First simultaneous multi-wavelength observations of the black hole candidate IGR J17091−3624" @default.
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• W4300882600 doi "https://doi.org/10.1051/0004-6361/201117511" @default.
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