A framework linking protostellar evolution tracks to radiative-transfer SED grids predicts that isothermal-sphere, turbulent-core, and competitive accretion histories produce distinct 100-micron and 3-millimeter flux signatures.
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A framework for modeling the evolution of young stellar objects
A framework linking protostellar evolution tracks to radiative-transfer SED grids predicts that isothermal-sphere, turbulent-core, and competitive accretion histories produce distinct 100-micron and 3-millimeter flux signatures.