Abstract We present high-resolution Very Large Array continuum observations at the S band (3 GHz, 560 pc scale) and X band (10 GHz, 200 pc scale) of the ram-pressure-stripped Virgo galaxy NGC 4522 to investigate the characteristics of its radio continuum, spectral index, and magnetic field under the influence of the intracluster medium (ICM). The total radio continuum shows an asymmetry that extends northwest, mirroring the H i gas distribution but showing distinct features in the extraplanar regions. The spectral index steepens systematically from α ∼ −0.6 in the main disk to α ∼ −1.1 in the outer disk. We find that the spectral index behavior of the outer disk is mainly due to an ICM shock that can reaccelerate electrons and a significant reduction of thermal emission. Intriguingly, extraplanar clouds exhibit exceptionally flat spectral indices ( α ∼ −0.2 to 0), resulting from a combination of significantly enhanced thermal emission and pronounced spectral aging of the nonthermal component. Although some of these regions correlate with H α , others do not. We propose that the mixing between the ICM and interstellar medium (ISM) is an alternative mechanism that enhances thermal emission independently of star formation. Polarized continuum emissions are highly asymmetric, preferentially distributed along the ICM wind side, and the polarization fraction increases radially outward from the galactic midplane, indicating that the polarized emission is strongly influenced by the ICM wind. Our results show how and where the ICM substantially affects the ISM and also demonstrate that high-frequency observations are crucial for analyzing the radio continuum of ram pressure stripping galaxies.
Choi et al. (Thu,) studied this question.