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| Content Provider | EDP Sciences |
|---|---|
| Author | J. Rodriguez S. Corbel I. Caballero J. A. Tomsick T. Tzioumis A. Paizis M. Cadolle Bel E. Kuulkers |
| 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. |
| Page Count | 5 |
| File Format | HTM / HTML PDF |
| ISSN | 00046361 |
| Alternate Webpage(s) | https://www.aanda.org/articles/aa/abs/2011/09/aa17511-11/aa17511-11.html |
| e-ISSN | 14320746 |
| Journal | Astronomy & Astrophysics |
| Volume Number | 533 |
| DOI | 10.1051/0004-6361/201117511 |
| Language | English |
| Publisher | EDP Sciences |
| Publisher Date | 2011-09-01 |
| Access Restriction | Open |
| Rights Holder | © ESO, 2011 |
| Subject Keyword | accretion, accretion disks X-rays: binaries radio continuum: stars stars: individual: IGR J1709-8722;3624 accretion, accretion disks / X-rays: binaries / radio continuum: stars / stars: individual: IGR J1709-8722;3624 |
| Content Type | Text |
| Resource Type | Article |
| Subject | Astronomy and Astrophysics Space and Planetary Science |
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