ESO 371 25
(MWSC 1595)
0.81
UTI
0.79
CN
1.0
Cdens
0.75
CC3
0.75
Clit
1.0
Cdup
Radius (P>50% members)
1.9 [arcmin]
- CN 0.79 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.75 Well-studied
- Cdup 1.0 Unique
Overview
ESO 371 25 is a rich, very dense object of high C3 quality. Its parallax locates it at a large distance, well above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, old cluster (see Parameters). It is well-studied in the literature.
Very distant
Moderate extinction
Near-solar metallicity
Old
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 133.248 | -35.477 | 0.147 | -2.398 | 1.79 | 37.439 |
| Hu & Soubiran | 2025 | 133.248 | -35.473 | â | â | â | â |
| Almeida et al. | 2025 | 133.249 | -35.471 | â | â | â | â |
| Hunt & Reffert | 2024 | 133.247 | -35.479 | 0.157 | -2.393 | 1.787 | 36.453 |
| Cavallo et al. | 2024 | 133.248 | -35.473 | 0.157 | â | â | â |
| Hunt & Reffert | 2023 | 133.247 | -35.479 | 0.157 | -2.393 | 1.787 | 36.453 |
| Dias et al. | 2021 | 133.249 | -35.471 | 0.137 | -2.397 | 1.779 | â |
| Cantat-Gaudin et al. | 2020 | 133.248 | -35.476 | 0.134 | -2.429 | 1.749 | â |
| Cantat-Gaudin & Anders | 2020 | 133.248 | -35.476 | 0.134 | -2.429 | 1.749 | â |
| Soubiran et al. | 2018 | 133.248 | -35.476 | â | â | â | 48.91 |
| Bica et al. | 2019 | 133.245 | -35.48 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 133.248 | -35.476 | 0.134 | -2.429 | 1.749 | â |
| Dias et al. | 2014 | 133.25 | -35.477 | â | -5.84 | 2.95 | â |
| Dias et al. | 2002 | 133.25 | -35.477 | â | -5.84 | 2.95 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Hu & Soubiran | 2025 | â | â | â | â | -0.140* | â | â | â |
| Almeida et al. | 2025 | 5.63 | 1.46 | â | 2716 | â | 933 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1000* | â | â |
| Cavallo et al. | 2024 | 4.68 | 1.26 | â | 3090 | -0.120 | â | â | â |
| Hunt & Reffert | 2023 | 5.59 | 1.56 | 0.55 | 995 | â | â | â | â |
| Dias et al. | 2021 | 5.63 | 1.46 | â | 2716 | -0.169 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 5.83 | 1.20 | â | 2042 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 6.11 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 6.11 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 6.11 | â | â | â | â | â | â | â |
| Dias et al. | 2002 | 2.20 | 0.84 | â | 3548 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: invalid due to poor quality CMD. Isochrone match: worst fit.
Cavallo et al. (2024)
Gold sample.