Constrained Local Group hydrodynamical simulations predict up to 8 HI-detectable dark galaxies within 2.5 Mpc of the Milky Way.
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Higher-resolution spectra reveal outflow signatures in ~30% of low-mass galaxies (rising to ~60% at higher SFR), with ionized mass outflow rates of 0.1-50 x 10^-3 solar masses per year.
Hydrodynamical simulations demonstrate that classical bulges enable bar-driven formation of nuclear stellar disks that bifurcate into pressure-supported nuclear star clusters and rotationally-supported nuclear stellar rings after gas depletion.
The TNG50-SKIRT Atlas shows that nonparametric galaxy morphology indicators vary significantly with wavelength, with stronger dependence in disc-dominated galaxies, while dust effects remain modest on average.
citing papers explorer
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HI-bearing dark galaxies predictions from constrained Local Group simulations: how many and where to find them
Constrained Local Group hydrodynamical simulations predict up to 8 HI-detectable dark galaxies within 2.5 Mpc of the Milky Way.
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Higher resolution optical spectra of $M_*<10^{10}~M_{\odot}$ galaxies reveal outflow signatures unresolved by the SDSS
Higher-resolution spectra reveal outflow signatures in ~30% of low-mass galaxies (rising to ~60% at higher SFR), with ionized mass outflow rates of 0.1-50 x 10^-3 solar masses per year.
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The SMUGGLE-Ring project: Bar and bulge effects on nuclear disk and ring formation
Hydrodynamical simulations demonstrate that classical bulges enable bar-driven formation of nuclear stellar disks that bifurcate into pressure-supported nuclear star clusters and rotationally-supported nuclear stellar rings after gas depletion.
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The TNG50-SKIRT Atlas: Multi-wavelength nonparametric galaxy morphology
The TNG50-SKIRT Atlas shows that nonparametric galaxy morphology indicators vary significantly with wavelength, with stronger dependence in disc-dominated galaxies, while dust effects remain modest on average.