Fast infrared variability from the black-hole candidate MAXI J1535571 and tight constraints on the modelling
arXiv:2102.06710 · doi:10.1093/mnras/stab475
Abstract
We present the results regarding the analysis of the fast X-ray/infrared (IR) variability of the black-hole transient MAXI J1535571. The data studied in this work consist of two strictly simultaneous observations performed with XMM-Newton (X-rays: 0.710 keV), VLT/HAWK-I ( band, 2.2 m) and VLT/VISIR ( and _ bands, 4.85 and 11.88 m respectively). The cross-correlation function between the X-ray and near-IR light curves shows a strong asymmetric anti-correlation dip at positive lags. We detect a near-IR QPO (2.5 ) at Hz simultaneously with an X-ray QPO at approximately the same frequency (). From the cross-spectral analysis a lag consistent with zero was measured between the two oscillations. We also measure a significant correlation between the average near-IR and mid-IR fluxes during the second night, but find no correlation on short timescales. We discuss these results in terms of the two main scenarios for fast IR variability (hot inflow and jet powered by internal shocks). In both cases, our preliminary modelling suggests the presence of a misalignment between disk and jet.
12 pages, 7 figures. Accepted for publication in MNRAS
References in corpus (23)
- The James Webb Space Telescope
- X-ray reverberation around accreting black holes
- Global General Relativistic MHD Simulation of a Tilted Black-Hole Accretion Disk
- ULTRACAM: an ultra-fast, triple-beam CCD camera for high-speed astrophysics
- Geometrical constraints on the origin of timing signals from black holes
- Discovery of oscillations above 200 keV in a black hole X-ray binary with Insight-HXMT
- Hot accretion flow in black hole binaries: a link connecting X-rays to the infrared
- A rapidly-changing jet orientation in the stellar-mass black hole V404 Cygni
- Rapid optical and X-ray timing observations of GX 339-4: flux correlations at the onset of a low/hard state
- The spectral energy distribution of compact jets powered by internal shocks
- Reflection Spectra of the Black Hole Binary Candidate MAXI J1535-571 in the Hard State Observed by NuSTAR
- AstroSat view of MAXI J1535-571: broadband spectro-temporal features
- SWIFT J1753.5-0127: a surprising optical/X-ray cross-correlation function
- Rapid compact jet quenching in the Galactic black hole candidate X-ray binary MAXI J1535-571
- Spectro-timing analysis of MAXI J1535-571 using AstroSat
- A Black Hole X-ray Binary at 100 Hz: Multiwavelength Timing of MAXI J1820+070 with HiPERCAM and NICER
- Multi-Wavelength Variability. Accretion and Ejection at the Fastest Timescales
- A unified accretion-ejection paradigm for black hole X-ray binaries. V. Low-frequency quasi-periodic oscillations
- Colours of black holes: infrared flares from the hot accretion disc in XTE J1550-564
- Can Lense-Thirring precession produce QPOs in supersonic accretion flows?
- The twisted jets of Circinus X-1
- Physical constraints from near-infrared fast photometry of the black-hole transient GX 339-4
- Sub-second variability in black-hole X-ray binary jets
Cited by in corpus (11)
- The Evolution of Rapid Optical/X-ray Timing Correlations in the Initial Hard State of MAXI J1820+070
- Are Low-Frequency Quasi-Periodic Oscillations seen in accretion flows the disk response to a jet instability?
- Wavelet analysis of MAXI J1535-571 with Insight-HXMT
- Black holes: Timing and spectral properties and evolution
- Wavelet analysis of the transient QPOs in MAXI J1535571 with Insight-HXMT
- Fast X-ray/IR observations of the black hole transient Swift~J1753.5--0127: from an IR lead to a very long jet lag
- The Accretion-Ejection Connection in the Black Hole X-ray Binary MAXI J1820070
- Tracking optical variability and outflows across the accretion states of the black hole transient MAXI J1820+070
- The simultaneity of emission from approaching and receding jets
- Optical and X-ray timing analysis of the 2018-2020 outburst and rebrightening of the black-hole transient MAXI J1820+070
- Rapid far-infrared spectral timing of X-ray binaries with PRIMA