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- W2600716963 abstract "Abstract Within the ‘earliest phases of star formation’ (EPoS) Herschel project, we observed the NH 3 inversion lines of 6 very young high-mass star-forming regions at high spatial resolution (3-5″) with the JVLA. While the Herschel data provide details about the dust continuum, the ammonia data reveal the kinematics and temperatures. Here we present the exciting star-forming clump ISOSS23053 that shows multiple velocity components. We observe a prominent velocity step within the clump, which could be a sign of colliding or converging flows that triggers star formation. Furthermore, we used the JVLA in the C-array configuration to study this source in more detail and we present the first results from the new data. They support the idea of converging flows, as we observe two components in the NH 3 (1,1) and (2,2) line, whereas the higher excited NH 3 (3,3) line shows one component that links the two lower excited lines." @default.
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- W2600716963 date "2015-08-01" @default.
- W2600716963 modified "2023-10-18" @default.
- W2600716963 title "Kinematic and thermal structure at the onset of high-mass star formation - ISOSS23053" @default.
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- W2600716963 doi "https://doi.org/10.1017/s1743921315010777" @default.
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