Double-peaked Lyα profiles during reionization require sightlines through nearby voids a few cMpc from the galaxy and a sufficiently strong local ionizing background, with occurrence probability rising sharply with background intensity.
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2 Pith papers cite this work. Polarity classification is still indexing.
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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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Double-Peaked Ly$\alpha$ Emission during Reionization Requires Nearby Voids and a Favorable Local Ionizing Background
Double-peaked Lyα profiles during reionization require sightlines through nearby voids a few cMpc from the galaxy and a sufficiently strong local ionizing background, with occurrence probability rising sharply with background intensity.
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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.