ESO 130 06

(MWSC 1998; FoF 2330)

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0.91 UTI
0.79
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
C3 classification AB
Number of members (P>50%) 203
Radius (P>50% members) 9.7 [arcmin]
  • CN 0.79 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 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
ℹī¸
ESO 130 06 is a rich, very dense object of high C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is very well-studied in the literature.
Close Low extinction Near-solar metallicity Intermediate age

Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit. Silver sample.

Cavallo et al. (2024)
Gold sample.

Data
🔍 Search references for ESO 130 06 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 – 181.97 -59.312 1.222 -11.29 -0.794 -7.236
Li et al. 2025 181.97 -59.31 1.229 -11.266 -0.866 –
Almeida et al. 2025 181.975 -59.308 – – – –
Alfonso et al. 2024 181.962 -59.312 1.194 -11.293 -0.801 –
Hunt & Reffert 2024 181.975 -59.31 1.22 -11.242 -0.775 -9.03
Cavallo et al. 2024 181.936 -59.303 1.233 – – –
Hunt & Reffert 2023 181.975 -59.31 1.22 -11.242 -0.775 -9.03
Almeida et al. 2023 181.991 -59.297 – – – –
Just et al. 2023 181.955 -59.297 – – – –
He et al. 2022 181.955 -59.317 1.23 -11.277 -0.804 –
Tarricq et al. 2022 181.979 -59.297 1.227 -11.31 -0.803 –
Dias et al. 2021 181.975 -59.308 1.23 -11.266 -0.862 –
Cantat-Gaudin et al. 2020 181.97 -59.31 1.229 -11.266 -0.866 –
Cantat-Gaudin & Anders 2020 181.97 -59.31 1.229 -11.266 -0.866 –
Liu & Pang 2019 181.99 -59.323 1.228 -11.255 -0.84 –
Soubiran et al. 2018 181.97 -59.31 – – – -5.68
Cantat-Gaudin et al. 2018 181.97 -59.31 1.229 -11.266 -0.866 –
Kharchenko et al. 2016 181.955 -59.297 – – – –
Dias et al. 2014 181.942 -59.3 – -7.65 -1.56 –
Kharchenko et al. 2013 181.965 -59.3 – -10.55 0.41 -1.0
Piskunov et al. 2008 181.933 -59.299 – – – –
Kharchenko et al. 2005 181.93 -59.3 – -10.8 -0.76 –

💡 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 0.84 0.34 – 204 0.234 – – –
Almeida et al. 2025 0.80 0.51 – 159 – 164 – –
Alfonso et al. 2024 0.81 0.27 – 207 0.057 – – –
Hunt & Reffert 2024 – – – – – 246* – –
Cavallo et al. 2024 0.77 0.22 – 363 0.350 – – –
Hunt & Reffert 2023 0.77 0.24 1.03 135 – – – –
Almeida et al. 2023 0.80 0.51 – 173 0.014 164* 0.43 –
Just et al. 2023 – – – 20 – 99 – –
He et al. 2022 – 0.65 – 112 – – – –
Tarricq et al. 2022 0.79 – – 151 – – – –
Dias et al. 2021 0.80 0.51 – 159 0.057 – – –
Cantat-Gaudin et al. 2020 0.81 0.27 – 141 – – – –
Cantat-Gaudin & Anders 2020 0.79 – – – – – – –
Liu & Pang 2019 – – – 33 0.250 – – –
Soubiran et al. 2018 0.79 – – – – – – –
Cantat-Gaudin et al. 2018 0.79 – – – – – – –
Kharchenko et al. 2016 1.20 1.03 – 20 – – – –
Kharchenko et al. 2013 1.20 1.03 – 20 -0.706 – – –
Piskunov et al. 2008 2.20 0.37 – 214 – – – –
Kharchenko et al. 2005 2.20 0.37 – 214 – – – –

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

Visualization
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ESO 130 06 UCC
ESO 130 06 HUNT23
ESO 130 06 CANTAT20
Galactocentric position diagram