Radio polarization and sub-mm observations of the Sombrero galaxy (NGC 4594) - Large-scale magnetic field configuration and dust emission

TL;DR

This study presents the first detection of a large-scale magnetic field in the Sa galaxy NGC 4594 (Sombrero galaxy) through radio polarization observations, revealing a disk-parallel magnetic field with vertical components and analyzing its dust content.

Contribution

It provides the first radio detection of a large-scale magnetic field in an Sa galaxy and characterizes its magnetic field configuration and dust properties.

Findings

Detected a large-scale magnetic field in NGC 4594.

Magnetic field is mainly parallel to the disk with vertical components.

Dust content is smaller than in more late-type spirals.

Abstract

We observed the nearby early-type spiral galaxy NGC 4594 (M 104, Sombrero galaxy) with the Very Large Array at 4.86 GHz, with the Effelsberg 100-m telescope at 8.35 GHz as well as with the Heinrich Hertz Telescope at 345 GHz in radio continuum. The 4.86 and 8.35 GHz data contain polarization information and hence information about the magnetic fields: we detected a large-scale magnetic field which is to our knowledge the first detection of a large-scale magnetic field in an Sa galaxy in the radio range. The magnetic field orientation in M104 is predominantly parallel to the disk but has also vertical components at larger z-distances from the disk. This field configuration is typical for normal edge-on spiral galaxies. The 345 GHz data pertain to the cold dust content of the galaxy. Despite the optical appearance of the object with the huge dust lane, its dust content is smaller than that of more late-type spirals.