In TNG50 Milky Way-like galaxies, ionized envelopes around high-velocity clouds carry about six times more mass than the neutral clouds and their infall rate is comparable to the galactic star formation rate.
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Invisible Accretion: Ionized Envelopes of TNG50 HVCs can Sustain Star Formation
In TNG50 Milky Way-like galaxies, ionized envelopes around high-velocity clouds carry about six times more mass than the neutral clouds and their infall rate is comparable to the galactic star formation rate.