Four infrared-selected young stellar objects are confirmed as FUor eruptions via CO and H2O absorption features, equivalent width diagrams, and disk models showing high extinction and accretion rates comparable to classical FUors.
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Characterizing and spectrally modeling embedded FUor eruptions in the near-infrared
Four infrared-selected young stellar objects are confirmed as FUor eruptions via CO and H2O absorption features, equivalent width diagrams, and disk models showing high extinction and accretion rates comparable to classical FUors.