NGC 6866
(MWSC 3239; FoF 2040)
0.97
UTI
0.84
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
21.3 [N/pc2]
- CN 0.84 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
NGC 6866 is a rich, very dense object of very high C3 quality. Its parallax locates it at a relatively 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 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 | 300.98 | 44.171 | 0.688 | -1.369 | -5.764 | 13.807 |
| Li et al. | 2025 | 300.983 | 44.158 | 0.686 | -1.365 | -5.743 | β |
| Hu & Soubiran | 2025 | 301.002 | 44.186 | β | β | β | β |
| Almeida et al. | 2025 | 300.983 | 44.16 | β | β | β | β |
| Zhang et al. | 2024 | 300.982 | 44.166 | β | β | β | β |
| Hunt & Reffert | 2024 | 300.982 | 44.166 | 0.692 | -1.372 | -5.764 | 15.177 |
| Cavallo et al. | 2024 | 301.002 | 44.186 | 0.69 | β | β | β |
| Hunt & Reffert | 2023 | 300.982 | 44.166 | 0.692 | -1.372 | -5.764 | 15.177 |
| Almeida et al. | 2023 | 300.971 | 44.16 | β | β | β | β |
| Just et al. | 2023 | 300.982 | 44.158 | β | β | β | β |
| Tarricq et al. | 2022 | 300.946 | 44.171 | 0.687 | -1.375 | -5.771 | β |
| Jaehnig et al. | 2021 | 300.986 | 44.164 | 0.716 | -1.379 | -5.737 | β |
| Rain et al. | 2021 | 300.983 | 44.158 | 0.686 | -1.365 | -5.743 | β |
| Dias et al. | 2021 | 300.983 | 44.16 | 0.686 | -1.358 | -5.733 | 13.519 |
| Cantat-Gaudin et al. | 2020 | 300.983 | 44.158 | 0.686 | -1.365 | -5.743 | β |
| SΓ‘nchez et al. | 2020 | 300.979 | 44.158 | β | -1.397 | -5.57 | β |
| Donor et al. | 2020 | 300.987 | 44.16 | β | -1.18 | -5.91 | 14.2 |
| Cantat-Gaudin & Anders | 2020 | 300.983 | 44.158 | 0.686 | -1.365 | -5.743 | β |
| Liu & Pang | 2019 | 301.0 | 44.188 | 0.683 | -1.411 | -5.748 | β |
| Bossini et al. | 2019 | 300.983 | 44.158 | β | β | β | β |
| Soubiran et al. | 2018 | 300.983 | 44.158 | β | β | β | 12.83 |
| Cantat-Gaudin et al. | 2018 | 300.983 | 44.158 | 0.686 | -1.365 | -5.743 | β |
| Loktin & Popova | 2017 | 300.975 | 44.158 | β | -2.022 | -3.143 | 13.7 |
| Kharchenko et al. | 2016 | 300.982 | 44.158 | β | β | β | β |
| Dias et al. | 2014 | 300.979 | 44.158 | β | -1.39 | -3.07 | β |
| Kharchenko et al. | 2013 | 300.987 | 44.16 | β | -2.75 | -4.8 | 13.7 |
| Gozha et al. | 2012 | 300.979 | 44.158 | β | β | β | β |
| Piskunov et al. | 2008 | 300.978 | 44.158 | β | β | β | β |
| van den Bergh | 2006 | 300.979 | 44.158 | β | β | β | β |
| Kharchenko et al. | 2005 | 300.97 | 44.16 | β | -3.48 | -5.8 | β |
| Kharchenko et al. | 2003 | 300.94 | 43.99 | β | -4.06 | -8.3 | β |
| Dias et al. | 2002 | 300.979 | 44.158 | β | -1.39 | -3.07 | 13.68 |
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 | 1.4 | 0.51 | 0.76 | 638 | 0.025 | 284 | 0.42 | 1.0 |
| Li et al. | 2025 | 1.36 | 0.39 | β | 848 | 0.039 | β | β | β |
| Hu & Soubiran | 2025 | β | β | β | β | -0.120(5) | β | β | β |
| Almeida et al. | 2025 | 1.35 | 0.50 | β | 726 | β | 284 | β | β |
| Zhang et al. | 2024 | β | β | β | β | -0.037(1) | β | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 1125(1) | β | β |
| Cavallo et al. | 2024 | 1.49 | 0.54 | β | 724 | 0.340 | β | β | β |
| Hunt & Reffert | 2023 | 1.39 | 0.31 | 0.76 | 630 | β | β | β | β |
| Almeida et al. | 2023 | 1.38 | 0.51 | β | 780 | 0.063 | 449(1) | 0.42 | β |
| Just et al. | 2023 | β | β | β | 437 | β | 94 | β | β |
| Tarricq et al. | 2022 | 1.36 | β | β | 646 | β | β | β | β |
| Jaehnig et al. | 2021 | 1.40(1) | β | β | β | β | β | β | β |
| Rain et al. | 2021 | 1.40 | 0.22 | β | 813 | β | β | β | 1 |
| Dias et al. | 2021 | 1.35 | 0.50 | β | 726 | 0.047 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 1.41 | 0.48 | β | 646 | β | β | β | β |
| Donor et al. | 2020 | β | β | β | β | 0.010 | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 1.40 | β | β | β | β | β | β | β |
| Liu & Pang | 2019 | β | β | β | 562 | 0.250 | β | β | β |
| Bossini et al. | 2019 | 1.34 | 0.40 | β | 776 | -0.013 | β | β | β |
| Soubiran et al. | 2018 | 1.40 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 1.40 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 1.47 | 0.52 | β | 389 | β | β | β | β |
| Kharchenko et al. | 2016 | 1.33 | 0.84 | β | 437 | β | β | β | β |
| Kharchenko et al. | 2013 | 1.33 | 0.84 | β | 437 | β | β | β | β |
| Gozha et al. | 2012 | 1.45 | β | β | 377 | β | 59 | β | β |
| Piskunov et al. | 2008 | 1.45 | 0.53 | β | 479 | β | β | β | β |
| van den Bergh | 2006 | 1.45 | 0.53 | β | 380 | β | β | β | β |
| Kharchenko et al. | 2005 | 1.45 | 0.53 | β | 479 | β | β | β | β |
| Kharchenko et al. | 2003 | 1.45 | 0.53 | β | β | β | β | β | β |
| Dias et al. | 2002 | 1.19 | 0.23 | β | 813 | -0.013 | 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: intermediate fit. Isochrone match: good fit.
Cavallo et al. (2024)
Gold sample.