2021
DOI: 10.48550/arxiv.2106.05615
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Rotating Motion of the Outflow of IRAS 16293-2422 A1 at its Origin Point near the Protostar

Yoko Oya,
Yoshimasa Watanabe,
Ana López-Sepulcre
et al.

Abstract: The Class 0 protostar IRAS 16293-2422 Source A is known to be a binary system (A1 and A2) or even a multiple system, which processes a complex outflow structure. We have observed this source in the C 34 S, SO, and OCS lines at 3.1 mm with the Atacama Large Millimeter/submillimeter Array (ALMA). A substructure of this source is traced by our high angular-resolution observation (0. ′′ 12; 20 au) of the continuum emission. The northwest-southeast (NW-SE) outflow on a 2 ′′ scale is detected in the SO (J N = 2 2 -1… Show more

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