ESO 392 13
(MWSC 2598)
0.72
UTI
0.4
CN
1.0
Cdens
1.0
CC3
0.6
Clit
1.0
Cdup
Radius (P>50% members)
7.7 [arcmin]
- CN 0.4 Poorly populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.6 Moderately studied
- Cdup 1.0 Unique
Overview
ESO 392 13 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age and mass parameters (see Parameters). It is moderately studied in the literature.
Relatively close
Moderate 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 | 261.702 | -34.717 | 0.924 | 1.649 | -2.848 | -26.58 |
| Almeida et al. | 2025 | 261.718 | -34.702 | â | â | â | â |
| Hunt & Reffert | 2024 | 261.683 | -34.744 | 0.922 | 1.664 | -2.84 | -26.608 |
| Cavallo et al. | 2024 | 261.702 | -34.721 | 0.922 | â | â | â |
| He et al. | 2023 | 261.691 | -34.73 | 0.927 | 1.648 | -2.843 | -55.78 |
| Hunt & Reffert | 2023 | 261.683 | -34.744 | 0.922 | 1.664 | -2.84 | -26.608 |
| Just et al. | 2023 | 261.708 | -34.683 | â | â | â | â |
| Dias et al. | 2021 | 261.718 | -34.702 | 0.9 | 1.69 | -2.882 | â |
| Kharchenko et al. | 2016 | 261.708 | -34.683 | â | â | â | â |
| Dias et al. | 2014 | 261.717 | -34.687 | â | -0.32 | 1.12 | â |
| Kharchenko et al. | 2013 | 261.717 | -34.683 | â | 0.29 | -1.2 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Almeida et al. | 2025 | 1.03 | 1.91 | â | 453 | â | 58 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 266* | â | â |
| Cavallo et al. | 2024 | 1.05 | 2.21 | â | 219 | 0.230 | â | â | â |
| He et al. | 2023 | 1.05 | 2.50 | â | 100 | â | â | â | â |
| Hunt & Reffert | 2023 | 1.04 | 2.20 | 1.58 | 109 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 89 | â | 23 | â | â |
| Dias et al. | 2021 | 1.03 | 1.91 | â | 453 | 0.074 | â | â | â |
| Kharchenko et al. | 2016 | 0.82 | 2.33 | â | 89 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.82 | 2.33 | â | 89 | 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: good fit.
Cavallo et al. (2024)
Gold sample.