SFUMATO# implements GPU-accelerated AMR for self-gravitational radiation hydrodynamics with new linearized implicit solvers for non-equilibrium chemistry and thermal evolution including dust.
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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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SFUMATO#: A GPU-accelerated code for self-gravitational radiation hydrodynamics simulation with adaptive mesh refinement
SFUMATO# implements GPU-accelerated AMR for self-gravitational radiation hydrodynamics with new linearized implicit solvers for non-equilibrium chemistry and thermal evolution including dust.
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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.