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.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
fields
astro-ph.GA 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
GMC clustering in galaxy disks is mostly set by large-scale galactic gas distribution, with stacked CO profiles showing an extended component beyond individual cloud sizes and stronger clustering around massive bound clouds.
citing papers explorer
-
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.
-
The Structure of Molecular Gas in PHANGS-ALMA Galaxies: Cloud Spacing, Two-Point Correlation and Stacked Intensity Profiles
GMC clustering in galaxy disks is mostly set by large-scale galactic gas distribution, with stacked CO profiles showing an extended component beyond individual cloud sizes and stronger clustering around massive bound clouds.