Jet kinematics in the transversely stratified jet of 3C 84 A two-decade overview
arXiv:2205.10281 · doi:10.1051/0004-6361/202243343
Abstract
3C84 (NGC1275) is one of the brightest radio sources in the mm radio-bands, which led to a plethora of VLBI observations at numerous frequencies over the years. They reveal a two-sided jet structure, with an expanding but not well-collimated parsec-scale jet, pointing southward. High resolution mm-VLBI observations allow the study and imaging of the jet base on the sub-parsec scale. This could facilitate the investigation of the nature of the jet origin, also in view of the previously detected two-railed jet structure and east-west oriented core region seen with RadioAstron at 22 GHz. We produce VLBI images of this core and inner jet region, observed during the past twenty years at 15, 43, and 86 GHz. We determine the kinematics of the inner jet and ejected features at 43 and 86 GHz and compare their ejection times with radio and -ray variability. For the moving jet features, we find an average velocity of c (mas/yr). From the time-averaged VLBI images at the three frequencies, we measure the transverse jet width along the bulk flow. On the parsec scale, we find a clear trend of the jet width being frequency dependent, with the jet being narrower at higher frequencies. This stratification is discussed in the context of a spine-sheath scenario, and is compared to other possible interpretations. From quasi-simultaneous observations at 43 and 86\,GHz we obtain spectral index maps, revealing a time-variable orientation of the spectral index gradient, due to structural variability of the inner jet.
23 pages, 12 figures, accepted for publication in A&A
References in corpus (20)
- Array Programming with NumPy
- MOJAVE: Monitoring of Jets in AGN with VLBA Experiments. V. Multi-epoch VLBA Images
- Magnetic acceleration of ultra-relativistic jets in gamma-ray burst sources
- Magnetic acceleration of relativistic AGN jets
- Kinematics of Parsec-Scale Jets of Gamma-Ray Blazars at 43~GHz within the VLBA-BU-BLAZAR Program
- MOJAVE: Monitoring of Jets in Active Galactic Nuclei with VLBA Experiments. VIII. Faraday rotation in parsec-scale AGN jets
- Kinematics of Parsec-Scale Jets of Gamma-Ray Bright Blazars at 43 GHz during Ten Years of the VLBA-BU-BLAZAR Program
- Jet collimation in NGC 315 and other nearby AGN
- Discovery of a new subparsec counterjet in NGC 1275: the inclination angle and the environment
- Wavelet-based decomposition and analysis of structural patterns in astronomical images
- A Non-thermal Study of the Brightest Cluster Galaxy NGC 1275 - The Gamma-Radio Connection Over Four Decades
- Enhanced Polarized Emission from the One-Parsec-Scale Hotspot of 3C 84 as a Result of the Interaction with Clumpy Ambient Medium
- GRMHD Simulations and Modeling for Jet Formation and Acceleration Region in AGNs
- Parsec Scale Faraday-Rotation Structure Across the Jets of 9 Active Galactic Nuclei
- Pinpointing the jet apex of 3C 84
- A detailed kinematic study of 3C 84 and its connection to Gamma-rays
- A persistent double nuclear structure in 3C 84
- Constraints on Circumnuclear Disk through Free-Free Absorption in the Nucleus of 3C 84 with KaVA and KVN at 43 and 86 GHz
- Observing the Time Evolution of the Multi-Component Nucleus of 3C\,84
- The Bulk Flow Velocity and Acceleration of the Inner Jet in M\,87
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- A multiband study and exploration of the radio wave - -ray connection in 3C 84
- Evidence for a toroidal magnetic field in the core of 3C 84
- Observational Evidence to Support a Dense Ambient Medium Shaping the Jet in 3C 84
- First VLBI detection of Fornax A
- Evolution, speed, and precession of the parsec-scale jet in the 3C 84 radio galaxy
- Detection of an orthogonal alignment between parsec scale AGN jets and their host galaxies
- Where within the 3C 84 jet are -rays produced?
- Detection of Compton scattering in the jet of 3C 84