HOPS 198
|
Distance (pc) |
Zone |
|||||||
|
0.7 |
61.4 |
0 |
386.0 |
LDN 1641 |
||||
|
ALMA 0.87 mm |
||||||||
|
Source |
||||||||
|
HOPS-198 |
05:35:22.196 |
-06:13:06.14 |
56.25 ± 1.64 |
10.41 |
0.32 |
0.3 |
0.41 x 0.07 |
158.4 |
|
VLA 9 mm |
||||||||
|
Source |
||||||||
|
HOPS-198 |
05:35:22.198 |
-06:13:06.16 |
0.217 ± 0.00 |
0.054 |
9.2 |
0.3 |
0.19 x 0.13 |
156.2 |
|
ACA 0.87 mm |
||||||||
|
Source |
||||||||
|
HOPS-198 |
05:35:22.176 |
-06:13:06.24 |
87.23 |
72.26 |
3.78 |
- |
- |
- |
ALMA and VLA Derived Parameters
|
Source |
||||||||
|
HOPS-198 |
134.1 ± 10.0 |
61.0 ± 10.0 |
63.5 ± 1.8 |
314.4 ± 0.0 |
7.91 |
1.93 |
2.4 ± 0.06 |
2.0 ± 0.0 |
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-198.
ALMA protostellar outflow survey (Hsieh et al. 2023).
Figure 2: HOPS-198 molecular outflows mass, momentum and energy maps (panels in the left column) and the corresponding rate maps (panels in the right column).