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- W3100448159 abstract "Massive molecular outflows erupting from high-mass young stellar objects (YSOs) provide important clues to understanding the mechanism of high-mass star formation. Based on new CO J = 3–2 and J = 1–0 observations using the Atacama Submillimeter Telescope Experiment (ASTE) and Mopra telescope facilities, we discovered a massive bipolar outflow associated with the dense dust core AGAL G337.916-00.477 (AGAL337.9-S), located 3.48 kpc from the Sun. The outflow lobes have extensions of less than 1 pc—and thus were not fully resolved in the angular resolutions of ASTE and Mopra—and masses of ∼50 M⊙. The maximum velocities of the outflow lobes are as high as 36–40 . Our analysis of the infrared and submillimeter data indicates that AGAL337.9-S is in an early evolutionary stage of high-mass star formation, having the total far-infrared luminosity of . We also found that another dust core, AGAL G337.922-00.456 (AGAL337.9-N), located 2' north of AGAL337.9-S, is a high-mass YSO in an earlier evolutionary stage than AGAL337.9-S, as it is less bright in the mid-infrared than AGAL337.9-S." @default.
- W3100448159 created "2020-11-23" @default.
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- W3100448159 date "2017-05-15" @default.
- W3100448159 modified "2023-10-18" @default.
- W3100448159 title "A Massive Molecular Outflow in the Dense Dust Core AGAL G337.916-00.477" @default.
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- W3100448159 doi "https://doi.org/10.3847/1538-4357/aa6fa8" @default.
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