VDBH 111

(vdB-Hagen 111; vdBergh-Hagen 111; MWSC 1901; BH 111; ESO 093 05)

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0.87 UTI
0.58
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
N50 (P>50% members) 66
Stellar density (N50/rad) 23.9 [N/pc2]
C3 classification AB
  • CN 0.58 Moderately populated
  • 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 MOCAMOCA 🔍 CDS 🔍 Simbad 🔍 CDS (Îą, δ) 🔍 Simbad (Îą, δ)

Overview
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VDBH 111 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the mass parameter (see Parameters). It is very well-studied in the literature.

Note: This object shares a moderate percentage of members with a later reported entry. See table with shared members information.

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

Cavallo et al. (2024)
Gold sample.

Data
🔍 Search references for VDBH 111 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 99999– 167.315 -63.834 0.367 -8.167 2.983 -66.23
Li et al. 2025 167.32 -63.834 0.339 -8.176 2.941 –
Almeida et al. 2025 167.314 -63.831 – – – –
Hunt & Reffert 2024 167.317 -63.83 0.367 -8.152 2.968 -66.434
Cavallo et al. 2024 167.326 -63.844 0.368 – – –
Hunt & Reffert 2023 167.317 -63.83 0.367 -8.152 2.968 -66.434
Just et al. 2023 167.272 -63.826 – – – –
Dias et al. 2021 167.314 -63.831 0.332 -8.164 2.935 –
Cantat-Gaudin et al. 2020 167.32 -63.834 0.339 -8.176 2.941 –
Cantat-Gaudin & Anders 2020 167.32 -63.834 0.339 -8.176 2.941 –
Bossini et al. 2019 167.32 -63.834 – – – –
Bica et al. 2019 167.28 -63.836 – – – –
Cantat-Gaudin et al. 2018 167.32 -63.834 0.339 -8.176 2.941 –
Kharchenko et al. 2016 167.272 -63.826 – – – –
Dias et al. 2014 167.283 -63.833 – -2.36 0.82 –
Kharchenko et al. 2013 167.28 -63.83 – -9.28 2.1 –
Piskunov et al. 2008 167.31 -63.831 – – – –
Kharchenko et al. 2005 167.31 -63.83 – -9.64 0.95 –
Kharchenko et al. 2003 167.35 -63.85 – -8.75 0.77 –
Dias et al. 2002 167.283 -63.833 – -8.75 0.77 –

💡 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 99999– 2.63 1.18 0.76 224 -0.064 301 – –
Li et al. 2025 2.30 1.18 – 734 -0.127 – – –
Almeida et al. 2025 2.48 1.44 – 326 – 172 – –
Hunt & Reffert 2024 – – – – – 301(1) – –
Cavallo et al. 2024 2.24 1.41 – 457 -0.160 – – –
Hunt & Reffert 2023 2.44 1.06 0.76 272 – – – –
Just et al. 2023 – – – 224 – 1406 – –
Dias et al. 2021 2.48 1.44 – 326 0.071 – – –
Cantat-Gaudin et al. 2020 2.84 1.28 – 195 – – – –
Cantat-Gaudin & Anders 2020 2.71 – – – – – – –
Bossini et al. 2019 2.58 1.09 – 274 0.000 – – –
Cantat-Gaudin et al. 2018 2.71 – – – – – – –
Kharchenko et al. 2016 2.63 1.29 – 224 – – – –
Kharchenko et al. 2013 2.63 1.29 – 224 – – – –
Piskunov et al. 2008 2.70 0.78 – 224 – – – –
Kharchenko et al. 2005 2.70 0.78 – 224 – – – –
Kharchenko et al. 2003 0.67 0.16 – – – – – –
Dias et al. 2002 2.70 0.78 – 224 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0561 45.5 167.32 -63.83 0.37 -8.19 2.98 – 0.0

💡 Note: The % column shows the percentage of members that VDBH 111 shares with each listed object.

Visualization
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VDBH 111 UCC
VDBH 111 HUNT23
VDBH 111 CANTAT20
Galactocentric position diagram