The MHONGOOSE survey obtained ultra-deep 21-cm neutral hydrogen (HI) observations with the MeerKAT radio telescope to map the distribution and kinematics of low-column-density gas in and around 30 nearby star-forming spiral and dwarf galaxies. MHONGOOSE routinely reaches its target HI column-density sensitivity of a few times 10^{17} atoms cm^{-2}, two orders of magnitude below the typical column densities found in galaxy HI disks.
These extremely deep resolved HI observations of nearby galaxies show that the outskirts of disk galaxies are complex and dynamic environments, with many potential accretion and interaction features visible in HI that have only now become detectable thanks to MeerKAT's excellent column-density sensitivity.
MHONGOOSE provides unique constraints on the role of cold gas in replenishing the gas reservoirs of nearby galaxies, as shown by a first comparison of the MHONGOOSE observations with simulated HI maps from recent cosmological simulations, revealing marked differences in both morphology and kinematics and suggesting that cold-gas accretion may proceed more gently than predicted. I also discuss the unexpected variety in the shapes of the outer radial HI profiles and the relative importance of photoionisation and environment in shaping the outer HI disks.
The sensitive MHONGOOSE observations point the way towards a better understanding of the role of gas accretion in galaxy evolution in the nearby Universe and highlight opportunities for future HI surveys with the upcoming SKA-MID telescope.