Multifrequency VLA observations of the FR I radio galaxy 3C 31: morphology, spectrum and magnetic field
arXiv:0803.2597 · doi:10.1111/j.1365-2966.2008.13091.x
Abstract
We present high-quality VLA images of the FR I radio galaxy 3C 31 in the frequency range 1365 to 8440 MHz with angular resolutions from 0.25 to 40 arcsec. Our new images reveal complex, well resolved filamentary substructure in the radio jets and tails. We also use these images to explore the spectral structure of 3C 31 on large and small scales. We infer the apparent magnetic field structure by correcting for Faraday rotation. Some of the intensity substructure in the jets is clearly related to structure in their apparent magnetic field: there are arcs of emission where the degree of linear polarization increases, with the apparent magnetic field parallel to the ridges of the arcs. The spectral indices are significantly steeper (0.62) within 7 arcsec of the nucleus than between 7 and 50 arcsec (0.52 - 0.57). The spectra of the jet edges are also slightly flatter than the average for their surroundings. At larger distances, the jets are clearly delimited from surrounding larger-scale emission both by their flatter radio spectra and by sharp brightness gradients. The spectral index of 0.62 in the first 7 arcsec of 3C 31's jets is very close to that found in other FR I galaxies where their jets first brighten in the radio and where X-ray synchrotron emission is most prominent. Farther from the nucleus, where the spectra flatten, X-ray emission is fainter relative to the radio. The brightest X-ray emission from FR I jets is therefore not associated with the flattest radio spectra, but with a particle-acceleration process whose characteristic energy index is 2.24. The spectral flattening with distance from the nucleus occurs where our relativistic jet models require deceleration, and the flatter-spectra at the jet edges may be associated with transverse velocity shear. (Slightly abridged)
arXiv comment17 pages, 13 figures, accepted for publication in MNRAS
References in corpus (18)
- Particle acceleration at ultrarelativistic shocks: an eigenfunction method
- Relativistic models and the jet velocity field in the radio galaxy 3C 31
- Dynamical models for jet deceleration in the radio galaxy 3C 31
- A Chandra observation of the X-ray environment and jet of 3C31
- Radiation from the Relativistic Jet: a Role of the Shear Boundary Layer
- Chandra observations of the X-ray jet in 3C66B
- Shear acceleration in relativistic astrophysical jets
- Particle transport in tangled magnetic fields and Fermi acceleration at relativistic shocks
- New results on particle acceleration in the Centaurus A jet and counterjet from a deep Chandra observation
- The X-ray Jet in Centaurus A: Clues on the Jet Structure and Particle Acceleration
- Multifrequency observations of the jets in the radio galaxy NGC 315
- A relativistic model of the radio jets in NGC 315
- The inner jet of radio galaxy NGC 315 as observed with Chandra and the VLA
- A relativistic model of the radio jets in 3C 296
- Adiabatic relativistic models for the jets in the radio galaxy 3C 31
- A Chandra observation of the X-ray environment and jet of 3C296
- Canonical Particle Acceleration in FRI Radio Galaxies
- Coaxial Jets and Sheaths in Wide-Angle-Tail Radio Galaxies
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