MUSE-ALMA Haloes XV: Cold molecular, ionised, and stellar kinematics of HI-rich galaxies at z about 0.5

arXiv:2610.10113 · astro-ph.GA · Submitted 2026-10-07 · Read on arXiv

astro-ph.GA

Submitted: 2026-10-07

Updated: 2026-10-07

Terminology

• Velocity Dispersion — 61× in this paper · explained in 2 episodes
• Stellar Feedback — 8× in this paper · explained in 2 episodes
• Trace — 7× in this paper · explained in 2 episodes
• Consistency — 3× in this paper · explained in 3 episodes
• Metallicity — 3× in this paper · explained in 3 episodes
• European Research Council — 2× in this paper
• Anti-correlation — 1× in this paper · explained in 3 episodes
• Aperture — 1× in this paper · explained in 1 episode
• Calibration — 1× in this paper · explained in 7 episodes
• Cooperation — 1× in this paper · explained in 2 episodes
• Core — 1× in this paper · explained in 2 episodes
• European Space Agency — 1× in this paper
• Hubble Space Telescope — 1× in this paper
• Multi Unit Spectroscopic Explorer — 1× in this paper
• Very Large Telescope — 1× in this paper

Sources

• Stellar feedback SPICEs up [C II] emission in the first galaxies
• NOEMA3D: Resolving radial gas flows in disk galaxies at z~1.1-1.6 with high-resolution CO observations
• The Multi-Scale Multi-Phase Circumgalactic Medium: Observed and Simulated
• The MAGPI Survey: co-evolution of baryons and dark matter in star-forming disk-like galaxies at $0.1 \lesssim z \lesssim 0.85$

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