First look at the multiphase interstellar medium with synthetic observations of low-frequency Faraday tomography

TL;DR

This study uses synthetic low-frequency Faraday tomography observations from MHD simulations to analyze the contributions of different gas phases in the multiphase interstellar medium to polarized synchrotron emission, aiding interpretation of LOFAR data.

Contribution

It provides the first detailed numerical analysis linking multiphase ISM modeling with synthetic low-frequency polarization observations, enhancing understanding of observed Faraday rotation and synchrotron emission.

Findings

Both ionized and neutral gas phases significantly contribute to polarization signals.

The contribution of each phase depends on magnetic field orientation and line of sight.

Strong correlation between HI data and polarized intensity occurs when observing perpendicular to magnetic field.

Abstract

Faraday tomography of radio polarimetric data below 200 MHz from LOFAR are providing us with a new perspective on the diffuse and magnetized interstellar medium (ISM). Of particular interest is the discovery of Faraday-rotated synchrotron polarization associated with neutral gas, as traced by atomic hydrogen (HI) and dust. Here we present the first in-depth numerical study of these LOFAR results. We produce and analyze comprehensive synthetic observations of low-frequency synchrotron polarization from MHD simulations of colliding super shells in the multiphase ISM. We define five distinct gas phases over more than four orders of magnitude in gas temperature and density, ranging from hot, and warm, fully ionized gas to cold neutral medium. We focus on the contribution of each gas phase to synthetic observations of both rotation measure and synchrotron polarized intensity below 200 MHz. We also investigate the link between the latter and synthetic observations of optically thin HI gas. We find that, not only the fully ionized gas but also the warm partially ionized and neutral phases strongly contribute to the total rotation measure and polarized intensity. However, the contribution of each phase to the observables strongly depends on the choice of integration axis and the orientation of the mean magnetic field with respect to the shell-collision axis. Strong correlation between HI synthetic data and synchrotron polarized intensity, reminiscent of LOFAR results, is obtained with lines of sight perpendicular to the mean magnetic field direction. Our study suggests that multiphase modelling of MHD processes is needed in order to interpret observations of the radio sky at low frequency. This work is a first step toward understanding the complexity of low-frequency synchrotron emission that will be soon revolutionized by large-scale surveys with LOFAR and the SKA.