Westerlund 2
0.77
UTI
0.79
CN
1.0
Cdens
0.75
CC3
0.65
Clit
1.0
Cdup
Radius (P>50% members)
0.9 [arcmin]
- CN 0.79 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.65 Moderately studied
- Cdup 1.0 Unique
Overview
Westerlund 2 is a rich, very dense object of high C3 quality. Its parallax locates it at a large* distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, metal-rich, very young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~5.09 kpc) differs significantly from the median photometric distance (~2.85 kpc).
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
Relatively close
High extinction
Massive
Metal-rich
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 156.01 | -57.758 | 0.197 | -5.32 | 2.871 | 68.86 |
| Hunt & Reffert | 2024 | 156.003 | -57.756 | 0.192 | -5.352 | 2.879 | â |
| Celli et al. | 2024 | 155.992 | -57.764 | â | â | â | â |
| Cavallo et al. | 2024 | 156.008 | -57.756 | 0.192 | â | â | â |
| Hunt & Reffert | 2023 | 156.003 | -57.756 | 0.192 | -5.352 | 2.879 | â |
| Cantat-Gaudin et al. | 2020 | 156.01 | -57.758 | 0.209 | -5.246 | 2.895 | â |
| Cantat-Gaudin & Anders | 2020 | 156.01 | -57.758 | 0.209 | -5.246 | 2.895 | â |
| Cantat-Gaudin et al. | 2018 | 156.01 | -57.758 | 0.209 | -5.246 | 2.895 | â |
| Loktin & Popova | 2017 | 156.015 | -57.767 | â | -7.5 | 4.22 | â |
| Dias et al. | 2014 | 156.008 | -57.767 | â | -0.89 | 2.45 | â |
| van den Bergh | 2006 | 155.992 | -57.764 | â | â | â | â |
| Dias et al. | 2002 | 156.008 | -57.767 | â | -6.77 | 4.84 | â |
đĄ Note: The UCC values are estimated from its identified members.
| Reference | Year | Dist [kpc] | Av [mag] | DAv [mag] | Age [Myr] | [Fe/H] [dex] | Mass [Msun] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Hunt & Reffert | 2024 | â | â | â | â | â | 2390* | â | â |
| Celli et al. | 2024 | â | â | â | 4 | â | 2172 | â | â |
| Cavallo et al. | 2024 | 1.86 | 4.46 | â | 174 | 0.760 | â | â | â |
| Hunt & Reffert | 2023 | 5.41 | 4.52 | 3.03 | 76 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 4.21 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 4.21 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 1.92 | 2.32 | â | 21 | â | â | â | â |
| van den Bergh | 2006 | 1.87 | 2.42 | â | 17 | â | â | â | â |
| Dias et al. | 2002 | 2.85 | 5.12 | â | 2 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Silver sample.