Abstract
Aims. We aim to use the high spatial resolution of the Atacama Large Millimeter/submillimeter Array (ALMA) to map the flow pattern of molecular gas near DG Tauri and its disk, a young stellar object driving a jet and a molecular outflow. Methods. We use observations from ALMA in the J = 2-1 transition of 12CO, 13CO, and C 18O to study the Keplerian disk of DG Tauri and outflows that may be related to the disk and the jet. Results. We find a new wind component flowing radially at a steep angle (≈ 25° from the vertical) above the disk with a velocity of ≈ 3.1 km s -1. It continues the trend of decreasing velocity for increasing distance from the jet axis ("onion-like velocity structure"). Conclusions. The new component is located close to the protostellar disk surface and may be related to photoevaporative winds.
Original language | English |
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Article number | L1 |
Journal | Astronomy & Astrophysics |
Volume | 620 |
Early online date | 23 Nov 2018 |
DOIs | |
Publication status | Published - 1 Dec 2018 |
Keywords
- Outflows
- Protoplanetary disks
- Stars: Pre-main sequence
- Stars: Winds