The peculiar 2011 outburst of the black hole candidate IGR J17091-3624, a GRS 1915+105 like source?
arXiv:1202.6186 · doi:10.1111/j.1365-2966.2012.20834.x
Abstract
We report on the long-term monitoring campaign of the black hole candidate IGR J17091-3624 performed with INTEGRAL and Swift during the peculiar outburst started on January 2011. We have studied the two month spectral evolution of the source in detail. Unlike the previous outbursts, the initial transition from the hard to the soft state in 2011 was not followed by the standard spectral evolution expected for a transient black hole binary. IGR J17091-3624 showed pseudo periodic flare-like events in the light curve, closely resembling those observed from GRS 1915+105. We find evidence that these phenomena are due to the same physical instability process ascribed to GRS 1915+105. Finally we speculate that the faintness of IGR J17091-3624 could be not only due to the high distance of the source but to the high inclination angle of the system as well.
13 pages, 12 figures and 2 tables. Accepted for publication in MNRAS on 2012 February 28. Received in original form 2011 October 19
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- Determination of mass of IGR J17091-3624 from "Spectro-Temporal" variations during onset-phase of the 2011 outburst
- Why is IGR J17091-3624 so faint? Constraints on distance, mass, and spin from `phase-resolved' spectroscopy of the `heartbeat' oscillations
- Modified viscosity in accretion disks. Application to Galactic black hole binaries, intermediate mass black holes and AGN
- The INTEGRAL view on Black Hole X-ray Binaries
- Interplay between heartbeat oscillations and wind outflow in microquasar IGR J17091-3624
- Chaotic and stochastic processes in the accretion flows of the black hole X-ray binaries revealed by recurrence analysis
- An Atlas of Exotic Variability in IGR J17091-3624: A Comparison with GRS 1915+105
- The current state of disk wind observations in BHLMXBs through X-ray absorption lines in the iron band
- Spectral and Timing Properties of IGR J17091-3624 in the Rising Hard State During its 2016 Outburst
- The reflection component in the average and heartbeat spectra of the black-hole candidate IGR J17091-3642 during the 2016 outburst
- Observational aspects of Outbursting Black Hole Sources - Evolution of Spectro-Temporal features and X-ray Variability
- Broad-band spectral evolution and temporal variability of IGR J17091-3624 during its 2016 outburst : SWIFT and NuSTAR results
- AstroSat view of IGR J17091-3624 and GRS 1915+105: decoding the 'pulse' in the 'Heartbeat State'
- Discovery of a soft X-ray 8 mHz QPO from the accreting millisecond pulsar IGR J00291+5934
- Properties of unique hard X-ray dips observed from GRS 1915+105 and IGR J17091-3624 and their implications
- Detection of distinct power spectra in soft and hard X-ray bands in the hard state of GRS 1915+105
- A new variability pattern in GRS 1915+105 with NICER and Insight-HXMT observations
- Correlating nonlinear time series and spectral properties of IGR J17091-3624: Is it similar to GRS 1915+105?
- Swift/XRT, Chandra and XMM-Newton observations of IGR J17091-3624 as it returns into quiescence
- Similarities and Differences in Accretion Flow Properties between GRS 1915+105 and IGR J17091-3624: a Case Study
- Recurrent Instability in LMXB Accretion Disks: How Strange is GRS 1915+105?