ESO 393 15

(MWSC 2667)

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0.82 UTI
0.79
CN
1.0
Cdens
1.0
CC3
0.65
Clit
1.0
Cdup
Radius (P>50% members) 4.9 [arcmin]
  • CN 0.79 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.65 Moderately studied
  • Cdup 1.0 Unique

Overview

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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 and metallicity 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.

Relatively close High extinction Massive Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 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 –
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 – – –
Hunt & Reffert 2023 265.877 -34.219 0.384 0.696 -0.504 -13.008
Just et al. 2023 265.895 -34.214 – – – –
Cantat-Gaudin et al. 2020 265.923 -34.203 0.315 0.748 -0.489 –
Cantat-Gaudin & Anders 2020 265.923 -34.203 0.315 0.748 -0.489 –
Cantat-Gaudin et al. 2018 265.923 -34.203 0.315 0.748 -0.489 –
Kharchenko et al. 2016 265.895 -34.214 – – – –
Dias et al. 2014 265.888 -34.218 – -1.2 -2.4 –
Kharchenko et al. 2013 265.905 -34.213 – -9.15 0.23 –

💡 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
Li et al. 2025 1.75 2.33 – 370 0.053 – – –
Hunt & Reffert 2024 – – – – – 2220* – –
Cavallo et al. 2024 1.46 3.46 – 32 -1.010 – – –
Hunt & Reffert 2023 2.38 2.83 1.97 50 – – – –
Just et al. 2023 – – – 1413 – 243 – –
Cantat-Gaudin & Anders 2020 2.90 – – – – – – –
Cantat-Gaudin et al. 2018 2.90 – – – – – – –
Kharchenko et al. 2016 2.47 5.16 – 1413 – – – –
Kharchenko et al. 2013 2.47 5.16 – 1413 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 328 67.0 265.9 -34.21 0.38 0.7 -0.46 -11.92 0.0
OC 0698 15.1 265.89 -34.23 0.39 0.71 -0.45 7.8 0.0

💡 Note: The % column shows the percentage of members that ESO 393 15 shares with each listed object.

Visualization

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