Dark-matter-deficient dwarf galaxies form via tidal stripping of dark matter in interactions with massive companions

TL;DR

This study uses high-resolution cosmological simulations to show that tidal interactions with massive galaxies can strip dark matter from dwarf galaxies, explaining observed dark-matter-deficient dwarfs within the standard Lambda-CDM model.

Contribution

It demonstrates that dark matter stripping during galaxy interactions naturally produces dark-matter-deficient dwarfs, aligning simulation results with recent observations.

Findings

Approximately 30% of dwarfs show dark matter deficiency due to stripping.

10% of dwarfs have halo-to-stellar mass ratios below 10.

Most dark-matter-deficient dwarfs eventually merge with their hosts.

Abstract

In the standard Lambda-CDM paradigm, dwarf galaxies are expected to be dark-matter-rich, as baryonic feedback is thought to quickly drive gas out of their shallow potential wells and quench star formation at early epochs. Recent observations of local dwarfs with extremely low dark matter content appear to contradict this picture, potentially bringing the validity of the standard model into question. We use NewHorizon, a high-resolution cosmological simulation, to demonstrate that sustained stripping of dark matter, in tidal interactions between a massive galaxy and a dwarf satellite, naturally produces dwarfs that are dark-matter-deficient, even though their initial dark matter fractions are normal. The process of dark matter stripping is responsible for the large scatter in the halo-to-stellar mass relation in the dwarf regime. The degree of stripping is driven by the closeness of the orbit of the dwarf around its massive companion and, in extreme cases, produces dwarfs with halo-to-stellar mass ratios as low as unity, consistent with the findings of recent observational studies. ~30 per cent of dwarfs show some deviation from normal dark matter fractions due to dark matter stripping, with 10 per cent showing high levels of dark matter deficiency (Mhalo/M*<10). Given their close orbits, a significant fraction of dark-matter-deficient dwarfs merge with their massive companions (e.g. ~70 per cent merge over timescales of ~3.5 Gyrs), with the dark-matter-deficient population being constantly replenished by new interactions between dwarfs and massive companions. The creation of these galaxies is, therefore, a natural by-product of galaxy evolution and their existence is not in tension with the standard paradigm.