NGC 6939
(Melotte 231; Collinder 423; MWSC 3357; OCL 217; FSR 0315; FoF 640)
1.0
UTI
1.0
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
N50 (P>50% members)
1143
Stellar density (N50/rad)
56.1 [N/pc2]
- 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
Overview
NGC 6939 is a very rich, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, old 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.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999β | 307.919 | 60.653 | 0.522 | -1.82 | -5.459 | -19.096 |
| Bijavara Seshashayana et al. | 2025 | 307.721 | 60.61 | β | β | β | β |
| Li et al. | 2025 | 307.917 | 60.653 | 0.506 | -1.841 | -5.413 | β |
| Hu & Soubiran | 2025 | 307.932 | 60.657 | β | β | β | β |
| Wei et al. | 2025 | 307.924 | 60.651 | 0.525 | -1.819 | -5.454 | β |
| Carrasco-Varela et al. | 2025 | 307.968 | 60.689 | β | β | β | β |
| Almeida et al. | 2025 | 307.928 | 60.655 | β | β | β | β |
| Hunt & Reffert | 2024 | 307.901 | 60.651 | 0.525 | -1.817 | -5.462 | -18.805 |
| Cavallo et al. | 2024 | 307.932 | 60.657 | 0.525 | β | β | β |
| Hunt & Reffert | 2023 | 307.901 | 60.651 | 0.525 | -1.817 | -5.462 | -18.805 |
| Almeida et al. | 2023 | 307.937 | 60.65 | β | β | β | β |
| Just et al. | 2023 | 307.879 | 60.657 | β | β | β | β |
| Jadhav & Subramaniam | 2021 | 307.917 | 60.653 | β | β | β | β |
| Jaehnig et al. | 2021 | 307.914 | 60.655 | 0.54 | -1.845 | -5.42 | β |
| Rain et al. | 2021 | 307.917 | 60.653 | 0.506 | -1.841 | -5.413 | β |
| Dias et al. | 2021 | 307.928 | 60.655 | 0.506 | -1.838 | -5.41 | -18.775 |
| Cantat-Gaudin et al. | 2020 | 307.917 | 60.653 | 0.506 | -1.841 | -5.413 | β |
| SΓ‘nchez et al. | 2020 | 307.875 | 60.662 | β | -1.9 | -5.284 | β |
| Cantat-Gaudin & Anders | 2020 | 307.917 | 60.653 | 0.506 | -1.841 | -5.413 | β |
| Liu & Pang | 2019 | 307.919 | 60.648 | 0.508 | -1.845 | -5.408 | β |
| Soubiran et al. | 2018 | 307.917 | 60.653 | β | β | β | -18.99 |
| Bica et al. | 2019 | 307.817 | 60.63 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 307.917 | 60.653 | 0.506 | -1.841 | -5.413 | β |
| Loktin & Popova | 2017 | 307.875 | 60.662 | β | -0.67 | -0.41 | -42.0 |
| Kharchenko et al. | 2016 | 307.879 | 60.657 | β | β | β | β |
| Dias et al. | 2014 | 307.875 | 60.662 | β | -2.37 | -5.29 | β |
| Kharchenko et al. | 2013 | 307.882 | 60.66 | β | -2.07 | -1.35 | -42.0 |
| Gozha et al. | 2012 | 307.875 | 60.662 | β | β | β | β |
| Kharchenko et al. | 2012 | 307.882 | 60.66 | β | -2.13 | -1.34 | -42.0 |
| Bukowiecki et al. | 2011 | 307.875 | 60.66 | β | β | β | β |
| Kharchenko et al. | 2007 | 307.87 | 60.66 | β | 0.08 | β | β |
| Ahumada & Lapasset | 2007 | 307.875 | 60.667 | β | β | β | β |
| van den Bergh | 2006 | 307.875 | 60.662 | β | β | β | β |
| Chen et al. | 2003 | 307.879 | 60.657 | β | β | β | β |
| Dias et al. | 2002 | 307.875 | 60.662 | β | -2.37 | -5.29 | -42.0 |
| Lynga | 1987 | 307.857 | 60.641 | β | β | β | β |
| Sulentic et al. | 1973 | 307.85 | 60.635 | β | β | β | β |
π‘ 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 | 99999β | 1.8 | 1.01 | 1.29 | 1698 | 0.010 | 2959 | 0.59 | 4 |
| Bijavara Seshashayana et al. | 2025 | β | 0.85 | β | 1700 | -0.020(14) | β | β | β |
| Li et al. | 2025 | 1.73 | 1.29 | β | 1695 | -0.155 | β | β | β |
| Hu & Soubiran | 2025 | β | β | β | β | 0.050(5) | β | β | β |
| Wei et al. | 2025 | 2.24 | 1.11 | β | 1780 | 0.250 | 3101 | 0.59 | β |
| Carrasco-Varela et al. | 2025 | 1.76 | 0.92 | β | 1611 | 0.450 | β | β | 5(1) |
| Almeida et al. | 2025 | 1.76 | 0.92 | β | 1611 | β | 2306 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 5146(1) | β | β |
| Cavallo et al. | 2024 | 1.85 | 1.24 | β | 1259 | 0.300 | β | β | β |
| Hunt & Reffert | 2023 | 1.84 | 1.33 | 1.29 | 1050 | β | β | β | β |
| Almeida et al. | 2023 | 1.72 | 1.40 | β | 1524 | -0.007 | 2031(1) | 0.59 | β |
| Just et al. | 2023 | β | β | β | 1862 | β | 1219 | β | β |
| Spina et al. | 2022 | β | β | β | β | 0.105 | β | β | β |
| Jadhav & Subramaniam | 2021 | 1.82 | 0.85 | β | 1698 | β | 4526 | β | 3(1) |
| Jaehnig et al. | 2021 | 1.86(1) | β | β | β | β | β | β | β |
| Rain et al. | 2021 | 1.87 | 1.04 | β | 1585 | β | β | β | 2 |
| Dias et al. | 2021 | 1.76 | 0.92 | β | 1611 | 0.462 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 1.82 | 0.85 | β | 1698 | β | β | β | β |
| Kounkel et al. | 2020 | 1.80 | 1.24 | β | 1738 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 1.87 | β | β | β | β | β | β | β |
| Liu & Pang | 2019 | β | β | β | 1660 | 0.500 | β | β | β |
| Soubiran et al. | 2018 | 1.87 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 1.87 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 1.39 | 0.98 | β | 2183 | β | β | β | β |
| Kharchenko et al. | 2016 | 1.80 | 0.98 | β | 1862 | β | β | β | β |
| Kharchenko et al. | 2013 | 1.80 | 0.98 | β | 1862 | 0.000 | β | β | β |
| Bukowiecki et al. | 2012 | β | β | β | β | β | 2959 | β | β |
| Gozha et al. | 2012 | 1.80 | β | β | 1585 | 0.000 | β | β | β |
| Kharchenko et al. | 2012 | 1.80 | 0.98 | β | 1871 | 0.000 | β | β | β |
| Bukowiecki et al. | 2011 | 1.60(1) | 0.95 | β | 1413 | β | β | β | β |
| Ahumada & Lapasset | 2007 | β | 1.01 | β | 2239 | β | β | β | 5 |
| van den Bergh | 2006 | 1.19 | 1.01 | β | 2239 | β | β | β | β |
| Chen et al. | 2003 | 1.19 | 1.01 | β | 2210 | 0.020(1) | β | β | β |
| Dias et al. | 2002 | 1.80 | 1.04 | β | 1585 | 0.000 | β | β | β |
| Lynga | 1987 | 1.25 | 1.51 | β | 1820 | -0.110 | β | β | β |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit. Gold sample.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.99 (50th percentile).
Ahumada & Lapasset (2007)
Membership probabilities from (1985ChA&A...9..300Z): star 7, 98%; star 13, 97%; star 87, 86%; star 94, 99%. Stars 7 and 13 (2002AJ....124.2093R), and 59 and 349 (WEBDA) are cited as straggler candidates in (1969MNRAS.144..449C) and (1994AJ....108.1828M). Star 59 is also cited as a blue straggler in (1988PASP..100..338G), although is probably a non-member.