NGC 6067

(MWSC 2370; FoF 143)

Click to load Aladin Lite
1.0 UTI
1.0
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
N50 (P>50% members) 1131
Stellar density (N50/rad) 117.8 [N/pc2]
C3 classification AA
  • CN 1.0 Very rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 1.0 Very well-studied
  • Cdup 1.0 Unique
πŸ“₯ Members πŸ“Š Colab πŸ”¬ Bayestar19 MOCAMOCA πŸ” CDS πŸ” Simbad πŸ” CDS (Ξ±, Ξ΄) πŸ” Simbad (Ξ±, Ξ΄)

Overview
ℹ️
NGC 6067 is a very rich, very dense object of very 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 metallicity and mass parameters (see Parameters). It is very well-studied in the literature.

Note: This object contains blue stragglers according to at least one source.

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

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

Cavallo et al. (2024)
Gold sample.

Data
πŸ” Search references for NGC 6067 in: SciX Simbad
ℹ️
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 243.301 -54.231 0.469 -1.952 -2.579 -39.46
Li et al. 2025 243.299 -54.227 0.443 -1.907 -2.586 –
Wei et al. 2025 243.308 -54.232 0.469 -1.96 -2.58 –
Almeida et al. 2025 243.296 -54.226 – – – –
Hunt & Reffert 2024 243.295 -54.232 0.471 -1.961 -2.578 -38.778
Cavallo et al. 2024 243.301 -54.23 0.472 – – –
Hunt & Reffert 2023 243.295 -54.232 0.471 -1.961 -2.578 -38.778
Just et al. 2023 243.287 -54.219 – – – –
Jaehnig et al. 2021 243.301 -54.232 0.486 -1.903 -2.582 –
Rain et al. 2021 243.299 -54.227 0.443 -1.907 -2.586 –
Dias et al. 2021 243.296 -54.226 0.448 -1.908 -2.588 -38.814
Cantat-Gaudin et al. 2020 243.299 -54.227 0.443 -1.907 -2.586 –
SΓ‘nchez et al. 2020 243.296 -54.218 – -1.87 -2.561 –
Cantat-Gaudin & Anders 2020 243.299 -54.227 0.443 -1.907 -2.586 –
Liu & Pang 2019 243.298 -54.238 0.455 -1.902 -2.59 –
Soubiran et al. 2018 243.299 -54.227 – – – -38.9
Cantat-Gaudin et al. 2018 243.299 -54.227 0.443 -1.907 -2.586 –
Loktin & Popova 2017 243.3 -54.218 – -6.1 -10.589 -37.3
Kharchenko et al. 2016 243.287 -54.219 – – – –
Dias et al. 2014 243.296 -54.218 – -2.7 -5.78 –
Kharchenko et al. 2013 243.3 -54.22 – -2.0 -2.62 -37.3
Gozha et al. 2012 243.296 -54.218 – – – –
Piskunov et al. 2008 243.283 -54.218 – – – –
Kharchenko et al. 2007 243.3 -54.22 – 0.25 – -36.26
Piskunov et al. 2007 243.283 -54.218 – – – –
van den Bergh 2006 243.3 -54.217 – – – –
Kharchenko et al. 2005 243.3 -54.22 – -2.55 -2.39 -36.23
Kharchenko et al. 2003 243.28 -54.22 – -2.97 -1.84 –
Chen et al. 2003 243.333 -54.198 – -0.83 -2.47 -39.9
Dias et al. 2002 243.296 -54.218 – -2.75 -5.75 -39.99
Dambis 1999 243.296 -54.218 – – – –

πŸ’‘ 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– 1.79 1.18 0.68 110 0.130 893 0.34 2.0
Li et al. 2025 1.87 0.93 – 236 0.154 – – –
Wei et al. 2025 2.79 1.53 – 98 -0.250 4091 0.34 –
Almeida et al. 2025 1.79 1.20 – 127 – 3602 – –
Hunt & Reffert 2024 – – – – – 7332(1) – –
Cavallo et al. 2024 2.18 1.37 – 145 0.430 – – –
Hunt & Reffert 2023 1.96 0.99 0.68 89 – – – –
Just et al. 2023 – – – 93 – 553 – –
Jaehnig et al. 2021 2.10(1) – – – – – – –
Rain et al. 2021 2.12 1.18 – 117 – – – 2
Dias et al. 2021 1.79 1.20 – 127 0.089 – – –
Cantat-Gaudin et al. 2020 1.88 0.97 – 126 – – – –
Cantat-Gaudin & Anders 2020 2.12 – – – – – – –
Liu & Pang 2019 – – – 93 -0.250 – – –
Soubiran et al. 2018 2.12 – – – – – – –
Cantat-Gaudin et al. 2018 2.12 – – – – – – –
Loktin & Popova 2017 1.43 1.15 – 126 – – – –
Kharchenko et al. 2016 1.79 1.28 – 93 – – – –
Kharchenko et al. 2013 1.79 1.28 – 93 0.138 – – –
Gozha et al. 2012 1.42 – – 119 0.080 741 – –
Piskunov et al. 2008 1.42 1.24 – 102 – 893(1) – –
Piskunov et al. 2007 1.42 1.24 – 102 – 165 – –
van den Bergh 2006 1.42 1.18 – 120 – – – –
Kharchenko et al. 2005 1.42 1.24 – 102 – – – –
Kharchenko et al. 2003 1.42 1.18 – – – – – –
Chen et al. 2003 1.42 1.18 – 110 0.130(1) – – –
Dias et al. 2002 1.42 1.18 – 119 0.138 – – –
Dambis 1999 1.74 1.11 – 100 – – – –

(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 0642 2.1 243.43 -54.15 0.47 -1.89 -2.65 – 0.01

πŸ’‘ Note: The % column shows the percentage of members that NGC 6067 shares with each listed object.

Visualization
ℹ️
NGC 6067 UCC
NGC 6067 HUNT23
NGC 6067 CANTAT20
Galactocentric position diagram