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- W2316108510 abstract "Abstract Very Long Baseline Interferometry studies of different maser species observed at multiple epochs allow complementary measurements of the 3-dimensional velocity field of gas close (≲ 10 3 AU) to massive young stellar objects. Here, we review our recent results toward the high-mass star-forming region G23.01–0.41, where all the strongest molecular maser transitions known to date cluster within 2000 AU from the center of an hot molecular core and are associated with a so called extended green object. The overall maser kinematics reveals a common outflowing motion from a central object; the details of the spatial distribution and velocity field of each maser species hint at the presence of different dynamical structures: a collimated jet, a wide-angle wind, and a flattened rotating core. We further compare the simultaneous presence of maser emission from different molecular species with a recent evolutionary sequence for masers associated with massive young stellar objects." @default.
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- W2316108510 date "2012-01-01" @default.
- W2316108510 modified "2023-09-27" @default.
- W2316108510 title "VLBI maser kinematics in high-mass SFRs: G23.01–0.41" @default.
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- W2316108510 doi "https://doi.org/10.1017/s1743921312007363" @default.
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