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The Dark Matter Distributions in Low-Mass Disk Galaxies. II. The Inner Density Profiles

Relatores, NC; Newman, AB; Simon, JD; Ellis, R; Truong, P; Blitz, L; Bolatto, A; ... Neill, JD; + view all (2019) The Dark Matter Distributions in Low-Mass Disk Galaxies. II. The Inner Density Profiles. The Astrophysical Journal , 887 (1) , Article 94. 10.3847/1538-4357/ab5305. Green open access

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Abstract

Dark-matter-only simulations predict that dark matter halos have steep, cuspy inner density profiles, while observations of dwarf galaxies find a range of inner slopes that are often much shallower. There is debate whether this discrepancy can be explained by baryonic feedback or if it may require modified dark matter models. In Paper I of this series, we obtained high-resolution integral field Hα observations for 26 dwarf galaxies with M* = 108.1−109.7 M☉. We derived rotation curves from our observations, which we use here to construct mass models. We model the total mass distribution as the sum of a generalized Navarro–Frenk–White (NFW) dark matter halo and the stellar and gaseous components. Our analysis of the slope of the dark matter density profile focuses on the inner 300–800 pc, chosen based on the resolution of our data and the region resolved by modern hydrodynamical simulations. The inner slope measured using ionized and molecular gas tracers is consistent, and it is additionally robust to the choice of stellar mass-to-light ratio. We find a range of dark matter profiles, including both cored and cuspy slopes, with an average of r ~ -  r DM 0.74 0.07, shallower than the NFW profile, but steeper than those typically observed for lower-mass galaxies with M* ∼ 107.5 M☉. Simulations that reproduce the observed slopes in those lower-mass galaxies also produce slopes that are too shallow for galaxies in our mass range. We therefore conclude that supernova feedback models do not yet provide a fully satisfactory explanation for the observed trend in dark matter slopes.

Type: Article
Title: The Dark Matter Distributions in Low-Mass Disk Galaxies. II. The Inner Density Profiles
Open access status: An open access version is available from UCL Discovery
DOI: 10.3847/1538-4357/ab5305
Publisher version: https://doi.org/10.3847/1538-4357/ab5305
Language: English
Additional information: This version is the version of record. For information on re-use, please refer to the publisher’s terms and conditions.
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Physics and Astronomy
URI: https://discovery-pp.ucl.ac.uk/id/eprint/10086185
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