CHANG-ES. XXXVIII. A Thin Radio Halo Shaped by Slow Cosmic-Ray Transport in the Quiescent Galaxy NGC 4565
Authors:
Open Access
- 14 April 2026
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 1001 (2) , 164
Abstract
We present the Very Large Array C-array S -band (2–4 GHz) radio continuum observations of the nearby edge-on spiral galaxy NGC 4565, a target from the Continuum Halos in Nearby Galaxies—an EVLA Survey. We conduct rotation measure (RM) synthesis to probe the magnetic field structure and analyze the vertical radio continuum intensity profiles using the 1D cosmic-ray (CR) transportation models. The radio continuum emission of NGC 4565 is vertically compact, with a vertical-to-radial extent ratio of ∼1/6. Its vertical profile is optimally described by a two-component Gaussian distribution, yielding a mean Gaussian halo scale height of ∼3.0 kpc. The magnetic field is weak, predominantly disk parallel, with an equipartition strength of ≲5 μ G and an RM profile indicative of an axisymmetric spiral structure. Nevertheless, we identify a localized, faint vertical magnetic field component in the northeastern region, hinting at an X-shaped structure that spatially coincides with extraplanar structures detected in H i and soft X-ray emission. The CR transport modeling favors a flux-tube advection scenario, with a slow initial velocity of v 0 ≈ 60 km s −1 , consistent with a limited energy input from star formation. Therefore, the absence of an extended radio halo can be explained by the low star formation rate, the weak magnetic field, and the inefficient CR transport. The localized X-shaped field may trace a weak, magnetically guided outflow or a tidal perturbation induced by the nearby companion. NGC 4565 is thus a key quiescent benchmark for understanding the physical conditions required to drive large-scale outflows and generate extended radio halos.Keywords
All Related Versions
Funding Information
- MOST ∣ National Natural Science Foundation of China (12273036)
- MOST ∣ National Natural Science Foundation of China (12321003)
- MOST ∣ National Natural Science Foundation of China (12273111)
- MOST ∣ National Natural Science Foundation of China (12203098)
This publication has 83 references indexed in Scilit:
- Closing in on the origin of Galactic cosmic rays using multimessenger informationPhysics Reports, 2020
- Cool outflows in galaxies and their implicationsThe Astronomy and Astrophysics Review, 2020
- Discovery of massive star formation quenching by non-thermal effects in the centre of NGC 1097Nature Astronomy, 2017
- HI4PI: a full-sky H i survey based on EBHIS and GASSAstronomy & Astrophysics, 2016
- Magnetic fields in spiral galaxiesThe Astronomy and Astrophysics Review, 2015
- A new interpretation of the far-infrared – radio correlation and the expected breakdown at high redshiftAstronomy & Astrophysics, 2013
- A multi-scale multi-frequency deconvolution algorithm for synthesis imaging in radio interferometryAstronomy & Astrophysics, 2011
- The Westerbork Hydrogen Accretion in LOcal GAlaxieS (HALOGAS) surveyAstronomy & Astrophysics, 2011
- Cold gas accretion in galaxiesThe Astronomy and Astrophysics Review, 2008
- Revised equipartition and minimum energy formula for magnetic field strength estimates from radio synchrotron observationsAstronomische Nachrichten, 2005