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.
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VLBA astrometry measures parallaxes of 2.26-2.65 mas for YSOs in Orion, determining mean distances of 405 pc for NGC 2068, 403 pc for NGC 2024, 407 pc for sigma Orionis, 388.5 pc for the ONC, and 438 pc for L1641.
citing papers explorer
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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.
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Dynamical masses of YSOs with the VLBA: DYNAMO VLBA: Trigonometric parallaxes and proper motions of YSOs in Orion
VLBA astrometry measures parallaxes of 2.26-2.65 mas for YSOs in Orion, determining mean distances of 405 pc for NGC 2068, 403 pc for NGC 2024, 407 pc for sigma Orionis, 388.5 pc for the ONC, and 438 pc for L1641.