Revealing Multiple Nested Molecular Outflows with Rotating Signatures in HH270mms1-A with ALMA
We present molecular line observations of the protostellar outflow associated with HH270mms1 in the Orion B molecular cloud with ALMA. The ^12 CO ( J = 3−2) emissions show that the outflow velocity structure consists of four distinct components of low (≲10 km s ^−1 ), intermediate (∼10–25 km s ^−1 )...
| 發表在: | The Astrophysical Journal |
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| Main Authors: | , , |
| 格式: | Article |
| 語言: | 英语 |
| 出版: |
IOP Publishing
2024-01-01
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| 主題: | |
| 在線閱讀: | https://doi.org/10.3847/1538-4357/ad19ce |