Westerlund 2
Summary
Westerlund 2 is a rich, very dense object of high C3 quality. It is located at a large distance from the Sun, near the mid-plane. It is moderately studied in the literature.
This object shares a large percentage of members with a later reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dias et al. (2002) | 156.008 | -57.767 | – | -6.77 | 4.84 | – |
| Loktin & Popova (2017) | 156.015 | -57.767 | – | -7.5 | 4.22 | – |
| Cantat-Gaudin et al. (2018) | 156.01 | -57.758 | 0.209 | -5.246 | 2.895 | – |
| Cantat-Gaudin et al. (2020) | 156.01 | -57.758 | 0.209 | -5.246 | 2.895 | – |
| Hunt & Reffert (2023) | 156.003 | -57.756 | 0.192 | -5.352 | 2.879 | – |
| Cavallo et al. (2024) | 156.008 | -57.756 | 0.192 | – | – | – |
| Celli et al. (2024) | 155.992 | -57.764 | – | – | – | – |
| Hunt & Reffert (2024) | 156.003 | -57.756 | 0.192 | -5.352 | 2.879 | – |
| UCC | 156.01 | -57.758 | 0.197 | -5.32 | 2.871 | 68.86 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=1.65, Dist=2850.0, Age=6.3 |
| Loktin & Popova (2017) | E(B-V)=0.748, Dist=1920, logt=7.317 |
| Cantat-Gaudin et al. (2018) | dmode=4207.7 |
| Hunt & Reffert (2023) | AV50=4.518, diffAV50=3.026, MOD50=13.667, logAge50=7.88 |
| Cavallo et al. (2024) | AV50=4.46, dMod50=11.35, logAge50=8.24, [Fe/H]50=0.76 |
| Celli et al. (2024) | Age=4.0, Mc=2172.3 |
| Hunt & Reffert (2024) | MassJ=2389.55, MassTot=2465.59 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| Bica 417 | 78.8 | 156.01 | -57.76 | 0.19 | -5.35 | 2.86 | – | 0.03 |
