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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VLBA observations of Orion young stellar binaries yield Keplerian orbits and dynamical masses for four systems, with two showing agreement to SED-based estimates and one confirming an intermediate-mass star with nonthermal emission.
citing papers explorer
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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.
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Dynamical masses of young stellar objects with the VLBA: DYNAMO-VLBA: Radio binary stars in Orion
VLBA observations of Orion young stellar binaries yield Keplerian orbits and dynamical masses for four systems, with two showing agreement to SED-based estimates and one confirming an intermediate-mass star with nonthermal emission.