In post-processed RMHD simulations, the observationally reconstructed luminosity-to-mass ratio of star-forming clumps follows L/M ∝ SFE^1.20, independent of clump mass and initial conditions within the tested range.
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The Rosetta Stone Project. II. The correlation between star formation efficiency and L/M indicator for the evolutionary stages of star-forming clumps in post-processed radiative magnetohydrodynamics simulations
In post-processed RMHD simulations, the observationally reconstructed luminosity-to-mass ratio of star-forming clumps follows L/M ∝ SFE^1.20, independent of clump mass and initial conditions within the tested range.