ESO 559 13
(MWSC 1238)
0.73
UTI
0.29
CN
1.0
Cdens
0.38
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
1.9 [arcmin]
- CN 0.29 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.38 Low quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
ESO 559 13 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is very well-studied in the literature.
Relatively close
Low extinction
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 112.179 | -20.803 | 0.389 | -1.391 | 1.725 | 48.741 |
| Hu & Soubiran | 2025 | 112.184 | -20.8 | â | â | â | â |
| Almeida et al. | 2025 | 112.186 | -20.81 | â | â | â | â |
| Hunt & Reffert | 2024 | 112.178 | -20.802 | 0.4 | -1.399 | 1.715 | 48.735 |
| Cavallo et al. | 2024 | 112.184 | -20.8 | 0.4 | â | â | â |
| Hunt & Reffert | 2023 | 112.178 | -20.802 | 0.4 | -1.399 | 1.715 | 48.735 |
| Just et al. | 2023 | 112.171 | -20.808 | â | â | â | â |
| Dias et al. | 2021 | 112.186 | -20.81 | 0.401 | -1.396 | 1.713 | â |
| Cantat-Gaudin et al. | 2020 | 112.176 | -20.807 | 0.4 | -1.402 | 1.721 | â |
| Cantat-Gaudin & Anders | 2020 | 112.176 | -20.807 | 0.4 | -1.402 | 1.721 | â |
| Soubiran et al. | 2018 | 112.176 | -20.807 | â | â | â | 48.61 |
| Bica et al. | 2019 | 112.174 | -20.815 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 112.176 | -20.807 | 0.4 | -1.402 | 1.721 | â |
| Loktin & Popova | 2017 | 112.125 | -20.825 | â | -4.122 | 2.157 | â |
| Kharchenko et al. | 2016 | 112.171 | -20.808 | â | â | â | â |
| Dias et al. | 2014 | 112.175 | -20.825 | â | -2.03 | 0.35 | â |
| Kharchenko et al. | 2013 | 112.177 | -20.81 | â | -2.26 | -1.16 | â |
| Dias et al. | 2002 | 112.175 | -20.825 | â | -2.03 | 0.35 | 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 | -0.150* | â | â | â |
| Almeida et al. | 2025 | 2.25 | 1.07 | â | 578 | â | 90 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 127* | â | â |
| Cavallo et al. | 2024 | 2.38 | 1.11 | â | 676 | 0.130 | â | â | â |
| Hunt & Reffert | 2023 | 2.25 | 0.79 | 1.14 | 664 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 804 | â | 62 | â | â |
| Dias et al. | 2021 | 2.25 | 1.07 | â | 578 | 0.010 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.32 | 0.87 | â | 617 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.33 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 2.33 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.33 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 3.54 | 0.46 | â | 575 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.91 | 0.97 | â | 804 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.91 | 0.97 | â | 804 | â | â | â | â |
| Dias et al. | 2002 | 2.75 | 0.78 | â | 1000 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: worst fit. Isochrone match: intermediate fit.
Cavallo et al. (2024)
Gold sample.