HOPS 164
|
Distance (pc) |
Zone |
|||||||
|
0.5 |
50.0 |
0 |
385.0 |
LDN 1641 |
||||
|
ALMA 0.87 mm |
||||||||
|
Source |
||||||||
|
HOPS-164 |
05:37:00.425 |
-06:37:10.89 |
105.50 ± 2.24 |
29.12 |
0.46 |
0.6 |
0.22 x 0.14 |
150.8 |
|
VLA 9 mm |
||||||||
|
Source |
||||||||
|
HOPS-164 |
05:37:00.425 |
-06:37:10.91 |
0.592 ± 0.022 |
0.288 |
6.8 |
0.6 |
0.1 x 0.07 |
141.8 |
|
ACA 0.87 mm |
||||||||
|
Source |
||||||||
|
HOPS-164 |
05:37:00.456 |
-06:37:10.56 |
326.83 |
199.6 |
4.65 |
- |
- |
- |
ALMA and VLA Derived Parameters
|
Source |
||||||||
|
HOPS-164 |
70.6 ± 10.0 |
34.3 ± 10.0 |
133.5 ± 2.8 |
941.2 ± 35.0 |
5.06 |
0.79 |
2.2 ± 0.06 |
1.8 ± 0.33 |
Sources next/close to me: -
Same source, other names: -
Source Images
Left: ALMA (0.87 mm), Right: VLA (9 mm) (Tobin et al. 2020),
Bottom: ACA (0.87 mm) (Federman et al. 2022).
Figure 1: HOPS-164.
ALMA protostellar outflow survey (Hsieh et al. 2023).
Figure 2: HOPS-164 molecular outflows mass, momentum and energy maps (panels in the left column) and the corresponding rate maps (panels in the right column).