Resolved magnetic structures in the disk-halo interface of NGC 628
arXiv:1701.04829 · doi:10.1051/0004-6361/201629907
Abstract
Magnetic fields are essential to fully understand the interstellar medium (ISM) and its role in the disk-halo interface of galaxies is still poorly understood. Star formation is known to expel hot gas vertically into the halo and these outflows have important consequences for mean-field dynamo theory in that they can be efficient in removing magnetic helicity. We perform new observations of the nearby face-on spiral galaxy NGC 628 with the Karl G. Jansky Very Large Array (JVLA) at S-band and the Effelsberg 100-m telescope at frequencies of 2.6 GHz and 8.35 GHz. We obtain some of the most sensitive radio continuum images in both total and linearly polarised intensity of any external galaxy observed so far in addition to high-quality images of Faraday depth and polarisation angle from which we obtained evidence for drivers of magnetic turbulence in the disk-halo connection. Such drivers include a superbubble detected via a significant Faraday depth gradient coinciding with a HI hole. We observe an azimuthal periodic pattern in Faraday depth with a pattern wavelength of 3.7 0.1 kpc, indicating Parker instabilities. The lack of a significant anti-correlation between Faraday depth and magnetic pitch angle indicates that these loops are vertical in nature with little helical twisting, unlike in IC 342. We find that the magnetic pitch angle is systematically larger than the morphological pitch angle of the polarisation arms which gives evidence for the action of a large-scale dynamo where the regular magnetic field is not coupled to the gas flow and obtains a significant radial component. We additionally discover a lone region of ordered magnetic field to the north of the galaxy with a high degree of polarisation and a small pitch angle, a feature that has not been observed in any other galaxy so far and is possibly caused by an asymmetric HI hole.
25 pages, Accepted for publication in Astronomy and Astrophysics
References in corpus (20)
- High-Resolution Rotation Curves and Galaxy Mass Models from THINGS
- The GALEX Ultraviolet Atlas of Nearby Galaxies
- Multi-Scale CLEAN deconvolution of radio synthesis images
- Revised equipartition & minimum energy formula for magnetic field strength estimates from radio synchrotron observations
- Magnetism in the spiral galaxy NGC 6946: magnetic arms, depolarization rings, dynamo modes and helical fields
- HI holes and high-velocity clouds in the spiral galaxy NGC 6946
- Galactic dynamo and helicity losses through fountain flow
- Converting H Luminosities into Star Formation Rates
- Connecting Far-Infrared and Radio Morphologies of Disk Galaxies: Cosmic-Ray Electron Diffusion After Star Formation Episodes
- High-resolution radio continuum survey of M33 II. Thermal and nonthermal emission
- The nature of the low-frequency emission of M51: First observations of a nearby galaxy with LOFAR
- Magnetic fields in the nearby spiral galaxy IC 342: A multi-frequency radio polarization study
- The characteristic polarized radio continuum distribution of cluster spiral galaxies
- Discovery of a strong spiral magnetic field crossing the inner pseudoring of NGC 4736
- Synchrotron spectral index and interstellar medium densities of star-forming galaxies
- Magnetic Spiral Arms and Galactic Outflows
- Properties of the Magneto-ionic Medium in the Halo of M51 revealed by Wide-band Polarimetry
- High resolution radio continuum survey of M33: I. The radio maps
- The formation of regular interarm magnetic fields in spiral galaxies
- Faraday dispersion functions of galaxies
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- Magnetic fields and cosmic rays in M 31. I. Spectral indices, scale lengths, Faraday rotation, and magnetic field pattern
- Evolving Galactic Dynamos and Fits to the Reversing Rotation Measures in the Halo of NGC 4631
- PHANGS-JWST First Results: A combined HST and JWST analysis of the nuclear star cluster in NGC 628
- Multi-Phase Magnetic Fields in the Galaxy NGC 3627
- Understanding the secular evolution of NGC 628 using UVIT
- Connection of supernovae 2002ap, 2003gd, 2013ej, and 2019krl in M74 with atomic gas accretion and spiral structure
- Investigation of the Connection Between X-ray Binaries and Compact Star Clusters in NGC 628
- CHANG-ES XXXIV: a 20 kpc radio bubble in the halo of the star-forming galaxy NGC 4217
- Hot magnetic halo of NGC628 (M74)
- The role of magnetic fields in disc galaxies: spiral arm instability
- A new window into the sub-parsec scale magnetic field in the Milky Way? Unveiling small-scale magneto-ionic structures with Faraday complexity
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