Table 2
Median positions, proper motions, radial velocities, and the number of stars for the various subgroups in Lupus.
| Sample | α | δ | l | b | μαcosδ | μ δ | V r | Stars |
| (h:m:s) | (°′′′) | (°) | (°) | (mas/yr) | (mas/yr) | (km s-1) | ||
|
|
||||||||
| Lupus 1 | 15 46 42.1 | –35 00 46 | 338.8 | 15.3 | –14.0 | –21.1 | 2.5 ± 1.6 | 30 |
| Lupus 2 | 15 56 02.1 | –37 56 06 | 338.6 | 12.0 | –15.0 | –23.1 | 2.2 ± 0.9 | 15 |
| Lupus 3 | 16 08 53.2 | –39 05 34 | 339.5 | 9.4 | –12.0 | –20.4 | 1.0 ± 0.7 | 73 |
| Lupus 4 | 15 59 16.5 | –41 57 10 | 336.2 | 8.5 | –10.0 | –20.8 | 0.3 ± 3.8a | 9 |
|
|
||||||||
| Lupus (on-cloud) | 16 00 47.0 | –38 48 54 | 339.1 | 9.7 | –13.0 | –21.6 | 2.5 ± 0.4 | 160b |
| Lupus (off-cloud) | 15 12 39.8 | –40 50 52 | 329.9 | 14.0 | –20.0 | –21.8 | 4.6 ± 0.4 | 57 |
|
|
||||||||
| Lupus (full sample) | 15 49 30.7 | –38 59 48 | 338.2 | 11.0 | –16.0 | –21.7 | 3.7 ± 0.4 | 217 |
Notes. The uncertainties in the median proper motion values for each group are about 1–2 mas/yr.
The radial velocity value presented for Lupus 4 is based on only two stars and should be regarded with caution.
The number of stars in the Lupus star-forming clouds (Lupus 1–4) do not add to the total number of stars (160 stars) in the on-cloud population (see definition in Sect. 3.2), because those stars that are spread beyond the limits of these clouds (see 12CO intensity map in Fig. 3) were not assigned to any cloud.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.