Hot gas haloes around disc galaxies: O VII column densities from galaxy formation simulations

TL;DR

This study uses high-resolution galaxy formation simulations to predict O VII column densities in hot gas haloes around Milky Way-like galaxies, suggesting that upcoming observations could confirm these theoretical models.

Contribution

It provides detailed predictions of O VII column densities from simulated galaxy haloes, including the impact of the galactic disc, to guide future X-ray observational tests.

Findings

Predicted O VII column densities are just below current observational limits.

Including the galactic disc increases the estimated column densities.

Hot gas haloes around Milky Way-like galaxies are detectable with future observations.

Abstract

Numerical models of disc galaxy formation predict the existence of extended, hot ( T~10^6 K) gas haloes around present day spirals. The X-ray luminosity of these haloes is predicted to increase strongly with galaxy mass. However, searches for their X-ray emission have not been successful so far. We calculate the all sky O VII column density distributions for the haloes of three Milky Way like disc galaxies, resulting from cosmological high-resolution, N-body/gasdynamical simulations. We perform calculations both including the disc gas and without it, so the disc contribution to the column density is quantified. It is found that the column densities estimated for Milky Way-like galaxies are just below the observational upper limit, making a test of the hot halo paradigm likely within observational reach.