NGC 6067
(MWSC 2370; FoF 143)
Summary
NGC 6067 is a very rich, very dense object of very high C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It is very well-studied in the literature.
This object shares a very small percentage of members with a later reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dambis (1999) | 243.296 | -54.218 | – | – | – | – |
| Dias et al. (2002) | 243.296 | -54.218 | – | -2.75 | -5.75 | -39.99 |
| Chen et al. (2003) | 243.333 | -54.198 | – | -0.83 | -2.47 | -39.9 |
| Kharchenko et al. (2003) | 243.28 | -54.22 | – | -2.97 | -1.84 | – |
| Kharchenko et al. (2005) | 243.3 | -54.22 | – | -2.55 | -2.39 | -36.23 |
| Piskunov et al. (2007) | 243.283 | -54.218 | – | – | – | – |
| Kharchenko et al. (2007) | 243.3 | -54.22 | – | 0.25 | – | -36.26 |
| Piskunov et al. (2008) | 243.283 | -54.218 | – | – | – | – |
| Kharchenko et al. (2013) | 243.3 | -54.22 | – | -2.0 | -2.62 | -37.3 |
| Kharchenko et al. (2016) | 243.287 | -54.219 | – | – | – | – |
| Loktin & Popova (2017) | 243.3 | -54.218 | – | -6.1 | -10.589 | -37.3 |
| Cantat-Gaudin et al. (2018) | 243.299 | -54.227 | 0.443 | -1.907 | -2.586 | – |
| Soubiran et al. (2018) | 243.299 | -54.227 | – | – | – | -38.9 |
| Liu & Pang (2019) | 243.298 | -54.238 | 0.455 | -1.902 | -2.59 | – |
| Cantat-Gaudin et al. (2020) | 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 |
| Rain et al. (2021) | 243.299 | -54.227 | 0.443 | -1.907 | -2.586 | – |
| Jaehnig et al. (2021) | 243.301 | -54.232 | 0.486 | -1.903 | -2.582 | – |
| Just et al. (2023) | 243.287 | -54.219 | – | – | – | – |
| Hunt & Reffert (2023) | 243.295 | -54.232 | 0.471 | -1.961 | -2.578 | -38.778 |
| Cavallo et al. (2024) | 243.301 | -54.23 | 0.472 | – | – | – |
| Hunt & Reffert (2024) | 243.295 | -54.232 | 0.471 | -1.961 | -2.578 | -38.778 |
| Almeida et al. (2025) | 243.296 | -54.226 | – | – | – | – |
| UCC | 243.301 | -54.231 | 0.469 | -1.952 | -2.579 | -39.46 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dambis (1999) | E_B-V_=0.358, DM0=11.2, log_age_=8.0 |
| Dias et al. (2002) | E(B-V)=0.38, Dist=1417.0, Age=8.076, [Fe/H]=0.138 |
| Chen et al. (2003) | E(B-V)=0.38, HDis=1417, Age=0.11, [Fe/H]_1=0.13, [Fe/H]_2=0.02 |
| Kharchenko et al. (2003) | E(B-V)=0.38, Dist=1417 |
| Kharchenko et al. (2005) | E(B-V)=0.4, Dist=1417, logt=8.01 |
| Piskunov et al. (2007) | E(B-V)=0.4, Dist=1417, logt=8.01, logM=2.217 |
| Piskunov et al. (2008) | E(B-V)=0.4, Dist=1417, logt=8.01, logM=2.951, logMA=2.874 |
| Kharchenko et al. (2013) | E(B-V)=0.412, d=1793.0, logt=7.97, [Fe/H]=0.138 |
| Kharchenko et al. (2016) | E(B-V)=0.412, d=1793.0, logt=7.97 |
| Loktin & Popova (2017) | E(B-V)=0.37, Dist=1431, logt=8.099 |
| Cantat-Gaudin et al. (2018) | dmode=2120.6 |
| Soubiran et al. (2018) | dmode=2120.6 |
| Liu & Pang (2019) | Age=0.093, Z=-0.25 |
| Cantat-Gaudin et al. (2020) | AVNN=0.97, DistPc=1881.0, AgeNN=8.1 |
| Dias et al. (2021) | Av=1.198, Dist=1792, logage=8.105, [Fe/H]=0.089 |
| Rain et al. (2021) | E(B-V)=0.38, Dist=2120.6, log(Age)=8.07, NBSS=2 |
| Jaehnig et al. (2021) | dmode=2.104 |
| Just et al. (2023) | logt=7.97, logmt=2.743 |
| Hunt & Reffert (2023) | AV50=0.99, diffAV50=0.68, MOD50=11.457, logAge50=7.949 |
| Cavallo et al. (2024) | AV50=1.37, dMod50=11.69, logAge50=8.16, [Fe/H]50=0.43 |
| Hunt & Reffert (2024) | MassJ=7331.57, MassTot=7331.57 |
| Almeida et al. (2025) | AV=1.198, Dist=1792, logAge=8.105, MassRk=3601.5 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| OC 0642 | 2.1 | 243.43 | -54.15 | 0.47 | -1.89 | -2.65 | – | 0.01 |