Fast-rotating green valley galaxies maintain higher metallicities than slow-rotating ones because slow rotators experience stronger outflows and more mergers that deplete their chemical content.
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Constrained Local Group hydrodynamical simulations predict up to 8 HI-detectable dark galaxies within 2.5 Mpc of the Milky Way.
FUV imaging shows ongoing massive star formation in the extended low-density outskirts of NGC2090, with smaller complexes, rising specific SFR, and flux ratios consistent with a top-heavy IMF.
Hα survey of 357 ALFALFA LSBGs shows deviation from the Kennicutt-Schmidt law but adherence to the extended Schmidt law that includes stellar mass.
Star formation model choice in galaxy simulations controls giant molecular cloud lifetimes, yielding 20-30 Myr with sink particles versus over 200 Myr with the gravo-thermo-turbulent prescription.
citing papers explorer
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Contrasting evolutionary pathways of fast- and slow-rotating galaxies in the green valley
Fast-rotating green valley galaxies maintain higher metallicities than slow-rotating ones because slow rotators experience stronger outflows and more mergers that deplete their chemical content.
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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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Star Formation Beyond the Optical Disk : The Low-Density Outskirts of NGC2090
FUV imaging shows ongoing massive star formation in the extended low-density outskirts of NGC2090, with smaller complexes, rising specific SFR, and flux ratios consistent with a top-heavy IMF.
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An $\rm H\alpha$ Imaging Survey of the Low Surface Brightness Galaxies Selected from the Spring Sky Region of the 40% ALFALFA HI Survey
Hα survey of 357 ALFALFA LSBGs shows deviation from the Kennicutt-Schmidt law but adherence to the extended Schmidt law that includes stellar mass.
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From short-lived to long-lived clouds: impact of star formation models on giant molecular cloud evolution in simulations of an NGC 300-like galaxy
Star formation model choice in galaxy simulations controls giant molecular cloud lifetimes, yielding 20-30 Myr with sink particles versus over 200 Myr with the gravo-thermo-turbulent prescription.