ESO 368 14

(FSR 1343; MWSC 1339; MWSC 1338)

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0.92 UTI
0.57
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
C3 classification AA
Number of members (P>50%) 65
Radius (P>50% members) 1.5 [arcmin]
  • CN 0.57 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 1.0 Very well-studied
  • Cdup 1.0 Unique
đŸ“Ĩ Members 📊 Colab đŸ”Ŧ Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (Îą, δ) 🔍 Simbad (Îą, δ)

Overview
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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 age and mass parameters (see Parameters). It is very well-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.

Distant High extinction Near-solar metallicity Intermediate age

Almeida et al. (2025)
Mass determination: invalid due to poor quality CMD. Isochrone match: worst fit.

Cavallo et al. (2024)
Gold sample.

Data
🔍 Search references for ESO 368 14 in: SciX Simbad
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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 116.751 -32.962 0.262 -1.977 3.708 134.365
Almeida et al. 2025 116.758 -32.953 – – – –
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 – – –
Hunt & Reffert 2023 116.751 -32.963 0.252 -1.968 3.741 115.93
Just et al. 2023 116.773 -32.971 – – – –
Dias et al. 2021 116.758 -32.953 0.221 -1.871 3.654 –
Cantat-Gaudin et al. 2020 116.751 -32.959 0.222 -1.938 3.561 –
Cantat-Gaudin & Anders 2020 116.751 -32.959 0.222 -1.938 3.561 –
Monteiro & Dias 2019 116.751 -32.959 – -1.957 3.754 3.329
Soubiran et al. 2018 116.751 -32.959 – – – 45.62
Bica et al. 2019 116.761 -32.965 – – – –
Cantat-Gaudin et al. 2018 116.751 -32.959 0.222 -1.938 3.561 –
Loktin & Popova 2017 116.76 -32.968 – 4.18 6.702 –
Kharchenko et al. 2016 116.773 -32.971 – – – –
Dias et al. 2014 116.763 -32.968 – -3.76 1.15 –
Kharchenko et al. 2013 116.778 -32.973 – 2.65 4.5 –
Froebrich et al. 2007 116.763 -32.97 – – – –
Dias et al. 2002 116.763 -32.968 – -3.35 1.34 –

💡 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 3.37 3.31 – 172 – 401 – –
Hunt & Reffert 2024 – – – – – 779* – –
Cavallo et al. 2024 3.84 3.66 – 117 0.350 – – –
Hunt & Reffert 2023 3.32 3.80 1.66 97 – – – –
Just et al. 2023 – – – 447 – 7 – –
Dias et al. 2021 3.37 3.31 – 172 -0.100 – – –
Cantat-Gaudin et al. 2020 4.25 3.29 – 93 – – – –
Cantat-Gaudin & Anders 2020 3.99 – – – – – – –
Monteiro & Dias 2019 5.69 2.67 – 13 0.022 – – –
Soubiran et al. 2018 3.99 – – – – – – –
Cantat-Gaudin et al. 2018 3.99 – – – – – – –
Loktin & Popova 2017 3.99 3.01 – 7 – – – –
Kharchenko et al. 2016 1.27 1.29 – 447 – – – –
Kharchenko et al. 2013 1.27 1.29 – 447 – – – –
Dias et al. 2002 4.23 3.22 – 631 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0437 3.1 116.56 -32.86 0.29 -2.12 3.43 82.33 0.04

💡 Note: The % column shows the percentage of members that ESO 368 14 shares with each listed object.

Visualization
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ESO 368 14 UCC
ESO 368 14 HUNT23
ESO 368 14 CANTAT20
Galactocentric position diagram