Deep Radio Continuum Imaging of the Dwarf Irregular Galaxy IC 10: Tracing Star Formation and Magnetic Fields

We exploit the vastly increased sensitivity of the Expanded Very Large Array (EVLA) to study the radio continuum and polarization properties of the post– starburst, dwarf irregular galaxy IC10 at 6 cm, at a linear resolution of ∼ 50 pc. We find close agreement between radio continuum and Hα emission, from the brightest H II regions to the weaker emission in the disk. A quantitative analysis shows a strictly linear correlation, where the thermal component contributes 50% to the total radio emission, the remainder being due to a non–thermal component with a surprisingly steep radio spectral index of between −0.7 and −1.0 suggesting substantial radiation losses of the cosmic–ray electrons. We confirm and clearly resolve polarized emission at the 10 − 20% level associated with a non–thermal superbubble, where the ordered magnetic field is possibly enhanced due to the compression of the expanding bubble. A fraction of the cosmic–ray electrons has likely escaped because the measured radio emission is a factor of 3 lower than what is suggested by the Hα inferred SFR. Subject headings: galaxies: dwarf — galaxies: individual(IC 10) — galaxies: magnetic fields — radio continuum: galaxies