ESO 211 03
(FSR 1463; MWSC 1587; MWSC 1588)
0.82
UTI
0.85
CN
1.0
Cdens
0.75
CC3
0.74
Clit
1.0
Cdup
Nm (P>50%)
362
Core radius and density
2.4 [pc], 5.0 [pc-2]
- CN 0.85 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.74 Moderately studied
- Cdup 1.0 Unique
Overview
ESO 211 03 is a rich, very dense object of high C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, old cluster, but with a large variance across recent sources for the metallicity and mass parameters (see Parameters). It is moderately studied in the literature.
Note: This object contains blue stragglers according to at least one source.
Note: This object shares a very small percentage of members with 2 later reported entries. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999β | 132.894 | -50.254 | 0.176 | -4.686 | 4.388 | 64.642 |
| Li et al. | 2025 | 132.897 | -50.253 | 0.159 | -4.681 | 4.333 | β |
| Hu & Soubiran | 2025 | 132.895 | -50.256 | β | β | β | β |
| Almeida et al. | 2025 | 132.893 | -50.25 | β | β | β | β |
| Hunt & Reffert | 2024 | 132.9 | -50.254 | 0.176 | -4.681 | 4.408 | 73.403 |
| Cavallo et al. | 2024 | 132.895 | -50.256 | 0.171 | β | β | β |
| Hunt & Reffert | 2023 | 132.9 | -50.254 | 0.176 | -4.681 | 4.408 | 73.403 |
| Just et al. | 2023 | 132.896 | -50.242 | β | β | β | β |
| Jadhav & Subramaniam | 2021 | 132.897 | -50.253 | β | β | β | β |
| Dias et al. | 2021 | 132.893 | -50.25 | 0.161 | -4.695 | 4.339 | β |
| Cantat-Gaudin et al. | 2020 | 132.897 | -50.253 | 0.159 | -4.681 | 4.333 | β |
| SΓ‘nchez et al. | 2020 | 132.892 | -50.245 | β | -4.696 | 4.462 | β |
| Cantat-Gaudin & Anders | 2020 | 132.897 | -50.253 | 0.159 | -4.681 | 4.333 | β |
| Soubiran et al. | 2018 | 132.897 | -50.253 | β | β | β | 64.1 |
| Bica et al. | 2019 | 132.908 | -50.247 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 132.897 | -50.253 | 0.159 | -4.681 | 4.333 | β |
| Dias et al. | 2018 | β | β | β | -9.11 | 4.39 | β |
| Sampedro et al. | 2017 | 132.892 | -50.245 | β | -0.87 | 2.55 | β |
| Kharchenko et al. | 2016 | 132.896 | -50.242 | β | β | β | β |
| Dias et al. | 2014 | 132.892 | -50.245 | β | -2.91 | 4.4 | β |
| Kharchenko et al. | 2013 | 132.9 | -50.245 | β | -2.38 | 6.12 | β |
| Bukowiecki et al. | 2011 | 132.933 | -50.244 | β | β | β | β |
| Glushkova et al. | 2010 | 132.893 | -50.245 | β | β | β | β |
| Froebrich et al. | 2007 | 132.925 | -50.243 | β | β | β | β |
| Dias et al. | 2002 | 132.892 | -50.245 | β | -2.91 | 4.4 | β |
π‘ 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999β | 4.91 | 3.13 | 1.99 | 1084 | -0.059 | 3359 | β | 1 |
| Li et al. | 2025 | 6.03 | 2.95 | β | 922 | 0.439 | β | β | β |
| Hu & Soubiran | 2025 | β | β | β | β | -0.300(5) | β | β | β |
| Almeida et al. | 2025 | 5.69 | 3.13 | β | 780 | β | 2975 | β | β |
| Hunt & Reffert | 2024 | 4.91 | 3.40 | 1.99 | 441 | β | 3743(1) | β | β |
| Cavallo et al. | 2024 | 4.57 | 3.26 | β | 977 | -0.040 | β | β | β |
| Hunt & Reffert | 2023 | 4.91 | 3.40 | 1.99 | 441 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 1084 | β | 1146 | β | β |
| Jadhav & Subramaniam | 2021 | 5.32 | 2.59 | β | 1288 | β | 5000 | β | 1(1) |
| Dias et al. | 2021 | 5.69 | 3.13 | β | 780 | -0.077 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 5.32 | 2.59 | β | 1288 | β | β | β | β |
| Kounkel et al. | 2020 | 4.05 | 3.18 | β | 447 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 5.31 | β | β | β | β | β | β | β |
| Soubiran et al. | 2018 | 5.31 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 5.31 | β | β | β | β | β | β | β |
| Kharchenko et al. | 2016 | 4.27 | 3.42 | β | 1084 | β | β | β | β |
| Kharchenko et al. | 2013 | 4.27 | 3.42 | β | 1084 | β | β | β | β |
| Bukowiecki et al. | 2011 | 4.85(1) | 2.78 | β | 1122 | β | β | β | β |
| Glushkova et al. | 2010 | 3.77 | 2.84 | β | 1122 | β | β | β | β |
| Dias et al. | 2002 | 3.77 | 2.84 | β | 1122 | β | β | β | β |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit. Gold sample.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD classes: 0.46 (50th percentile), true positive (human-assigned).
Hunt & Reffert (2023)
Classified as open cluster. CMD classes: 0.46 (50th percentile), true positive (human-assigned).
Hu et al. (2021)
Ellipticities (core, all): e_core=0.0575, e_all=0.2635.