ESO 332 22
(MWSC 2537)
0.63
UTI
0.4
CN
1.0
Cdens
0.75
CC3
0.5
Clit
1.0
Cdup
Radius (P>50% members)
3.9 [arcmin]
- CN 0.4 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.5 Moderately studied
- Cdup 1.0 Unique
Overview
ESO 332 22 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is moderately studied in the literature.
Relatively close
High extinction
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 256.893 | -40.841 | 0.596 | -0.961 | -3.206 | â |
| Hunt & Reffert | 2024 | 256.878 | -40.842 | 0.602 | -0.943 | -3.196 | â |
| Cavallo et al. | 2024 | 256.881 | -40.846 | 0.602 | â | â | â |
| Hunt & Reffert | 2023 | 256.878 | -40.842 | 0.602 | -0.943 | -3.196 | â |
| Just et al. | 2023 | 256.843 | -40.818 | â | â | â | â |
| Bica et al. | 2019 | 256.877 | -40.817 | â | â | â | â |
| Kharchenko et al. | 2016 | 256.843 | -40.818 | â | â | â | â |
| Dias et al. | 2014 | 256.871 | -40.813 | â | 0.31 | -2.14 | â |
| Kharchenko et al. | 2013 | 256.852 | -40.817 | â | -3.72 | -2.69 | 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 | 317* | â | â |
| Cavallo et al. | 2024 | 1.56 | 2.80 | â | 398 | -0.230 | â | â | â |
| Hunt & Reffert | 2023 | 1.56 | 2.64 | 1.17 | 191 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 99 | â | 88 | â | â |
| Kharchenko et al. | 2016 | 1.42 | 3.23 | â | 99 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.42 | 3.23 | â | 99 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.