ESO 368 14
(FSR 1343; MWSC 1339; MWSC 1338)
0.80
UTI
0.57
CN
1.0
Cdens
1.0
CC3
0.71
Clit
1.0
Cdup
Nm (P>50%)
65
Core radius and density
0.8 [pc], 9.9 [pc-2]
- CN 0.57 Moderately populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.71 Moderately studied
- Cdup 1.0 Unique
Overview
ESO 368 14 is a moderately populated, 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 near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the distance, age, metallicity, and mass parameters (see Parameters). It is moderately studied in the literature.
Note: This object shares a very small percentage of members with a later reported entry. 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 | 116.751 | -32.962 | 0.262 | -1.977 | 3.708 | 134.365 |
| Almeida et al. | 2025 | 116.758 | -32.953 | â | â | â | â |
| Hunt & Reffert | 2024 | 116.751 | -32.963 | 0.252 | -1.968 | 3.741 | 115.93 |
| Cavallo et al. | 2024 | 116.753 | -32.968 | 0.254 | â | â | â |
| Hunt & Reffert | 2023 | 116.751 | -32.963 | 0.252 | -1.968 | 3.741 | 115.93 |
| Just et al. | 2023 | 116.773 | -32.971 | â | â | â | â |
| Dias et al. | 2021 | 116.758 | -32.953 | 0.221 | -1.871 | 3.654 | â |
| Cantat-Gaudin et al. | 2020 | 116.751 | -32.959 | 0.222 | -1.938 | 3.561 | â |
| Cantat-Gaudin & Anders | 2020 | 116.751 | -32.959 | 0.222 | -1.938 | 3.561 | â |
| Monteiro & Dias | 2019 | 116.751 | -32.959 | â | -1.957 | 3.754 | 3.329 |
| Soubiran et al. | 2018 | 116.751 | -32.959 | â | â | â | 45.62 |
| Bica et al. | 2019 | 116.761 | -32.965 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 116.751 | -32.959 | 0.222 | -1.938 | 3.561 | â |
| Dib et al. | 2018 | 116.778 | -32.973 | â | â | â | â |
| Loktin & Popova | 2017 | 116.76 | -32.968 | â | 4.18 | 6.702 | â |
| Sampedro et al. | 2017 | 116.763 | -32.97 | â | â | â | â |
| Joshi et al. | 2016 | 116.778 | -32.973 | â | â | â | â |
| Kharchenko et al. | 2016 | 116.773 | -32.971 | â | â | â | â |
| Dias et al. | 2014 | 116.763 | -32.968 | â | -3.76 | 1.15 | â |
| Kharchenko et al. | 2013 | 116.778 | -32.973 | â | 2.65 | 4.5 | â |
| Bukowiecki et al. | 2011 | 116.746 | -32.97 | â | â | â | â |
| Froebrich et al. | 2007 | 116.763 | -32.97 | â | â | â | â |
| Dias et al. | 2002 | 116.763 | -32.968 | â | -3.35 | 1.34 | 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 | 3.87 | 3.19 | 1.66 | 172 | 0.022 | 401 | â | â |
| Liu et al. | 2025 | 15.07 | 1.31 | â | 100 | â | â | â | â |
| Almeida et al. | 2025 | 3.37 | 3.31 | â | 172 | â | 401 | â | â |
| Hunt & Reffert | 2024 | 3.32 | 3.80 | 1.66 | 97 | â | 779(1) | â | â |
| Cavallo et al. | 2024 | 3.84 | 3.66 | â | 117 | 0.350 | â | â | â |
| Hunt & Reffert | 2023 | 3.32 | 3.80 | 1.66 | 97 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 447 | â | 7 | â | â |
| Dias et al. | 2021 | 3.37 | 3.31 | â | 172 | -0.100 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 4.25 | 3.29 | â | 93 | â | â | â | â |
| Kounkel et al. | 2020 | 3.87 | 2.89 | â | 955 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 3.99 | â | â | â | â | â | â | â |
| Monteiro & Dias | 2019 | 5.69 | 2.71 | â | 13 | 0.022 | â | â | â |
| Soubiran et al. | 2018 | 3.99 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 3.99 | â | â | â | â | â | â | â |
| Dib et al. | 2018 | 1.27 | â | â | 447 | â | â | â | â |
| Loktin & Popova | 2017 | 3.99 | 3.06 | â | 7 | â | â | â | â |
| Joshi et al. | 2016 | 1.27 | 1.31 | â | 447 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.27 | 1.31 | â | 447 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.27 | 1.31 | â | 447 | â | â | â | â |
| Bukowiecki et al. | 2011 | 4.28(1) | 3.19 | â | 631 | â | â | â | â |
| Dias et al. | 2002 | 4.23 | 3.28 | â | 631 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Liu et al. (2025)
Classified as tidal capture (resonant trapping binary) 260 along with Haffner_15.
Palma et al. (2025)
Part of multiple system G73, along with HSC_1999 and Haffner_15.
Almeida et al. (2025)
Mass determination: invalid due to poor quality CMD. Isochrone match: worst fit.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.95 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.95 (50th percentile).
Hu et al. (2021)
Ellipticities (core, all): e_core=0.0954, e_all=0.0245.