Protostellar luminosities can be estimated from single or few infrared photometric measurements at 40-350 microns with 1-sigma uncertainties of factors 2-3 using evolutionary radiative transfer models.
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Estimating the Luminosities of Protostars with Limited Infrared Photometry
Protostellar luminosities can be estimated from single or few infrared photometric measurements at 40-350 microns with 1-sigma uncertainties of factors 2-3 using evolutionary radiative transfer models.