ESO 393 15
(MWSC 2667)
0.80
UTI
0.79
CN
1.0
Cdens
1.0
CC3
0.6
Clit
1.0
Cdup
Stellar density (N50/rad)
14.6 [N/pc2]
- CN 0.79 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.6 Moderately studied
- Cdup 1.0 Unique
Overview
ESO 393 15 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age, metallicity, and mass parameters (see Parameters). It is moderately studied in the literature.
Note: This object shares a significant 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 | 99999â | 265.902 | -34.211 | 0.369 | 0.707 | -0.464 | -11.918 |
| Li et al. | 2025 | 265.923 | -34.203 | 0.315 | 0.748 | -0.489 | â |
| Hunt & Reffert | 2024 | 265.877 | -34.219 | 0.384 | 0.696 | -0.504 | -13.008 |
| Cavallo et al. | 2024 | 265.908 | -34.219 | 0.382 | â | â | â |
| Hunt & Reffert | 2023 | 265.877 | -34.219 | 0.384 | 0.696 | -0.504 | -13.008 |
| Just et al. | 2023 | 265.895 | -34.214 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 265.923 | -34.203 | 0.315 | 0.748 | -0.489 | â |
| Cantat-Gaudin & Anders | 2020 | 265.923 | -34.203 | 0.315 | 0.748 | -0.489 | â |
| Cantat-Gaudin et al. | 2018 | 265.923 | -34.203 | 0.315 | 0.748 | -0.489 | â |
| Kharchenko et al. | 2016 | 265.895 | -34.214 | â | â | â | â |
| Dias et al. | 2014 | 265.888 | -34.218 | â | -1.2 | -2.4 | â |
| Kharchenko et al. | 2013 | 265.905 | -34.213 | â | -9.15 | 0.23 | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 2.47 | 3.46 | 1.97 | 892 | -0.478 | 1232 | â | â |
| Li et al. | 2025 | 1.75 | 2.33 | â | 370 | 0.053 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 2220(1) | â | â |
| Cavallo et al. | 2024 | 1.46 | 3.46 | â | 32 | -1.010 | â | â | â |
| Hunt & Reffert | 2023 | 2.38 | 2.83 | 1.97 | 50 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 1413 | â | 243 | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.90 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.90 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 2.47 | 5.16 | â | 1413 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.47 | 5.16 | â | 1413 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Gold sample.