NGC 6991
(FoF 2342)
0.97
UTI
0.85
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
18.9 [N/pc2]
- CN 0.85 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
NGC 6991 is a rich, very dense object of very high C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, old cluster (see Parameters). It is very well-studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 313.61 | 47.379 | 1.769 | 5.616 | 8.422 | -12.222 |
| Li et al. | 2025 | 313.621 | 47.4 | 1.765 | 5.593 | 8.509 | â |
| Hu & Soubiran | 2025 | 313.638 | 47.422 | â | â | â | â |
| Wei et al. | 2025 | 313.582 | 47.345 | 1.771 | 5.564 | 8.397 | â |
| Almeida et al. | 2025 | 313.689 | 47.405 | â | â | â | â |
| Alfonso et al. | 2024 | 313.608 | 47.395 | 1.741 | 5.614 | 8.415 | â |
| Hunt & Reffert | 2024 | 313.649 | 47.377 | 1.767 | 5.604 | 8.436 | -12.326 |
| Cavallo et al. | 2024 | 313.638 | 47.422 | 1.769 | â | â | â |
| Hunt & Reffert | 2023 | 313.649 | 47.377 | 1.767 | 5.604 | 8.436 | -12.326 |
| Almeida et al. | 2023 | 313.798 | 47.269 | â | â | â | â |
| He et al. | 2022 | 313.655 | 47.395 | 1.771 | 5.622 | 8.402 | â |
| Tarricq et al. | 2022 | 313.631 | 47.43 | 1.775 | 5.617 | 8.392 | â |
| Dias et al. | 2021 | 313.689 | 47.405 | 1.766 | 5.589 | 8.505 | -12.027 |
| Cantat-Gaudin et al. | 2020 | 313.621 | 47.4 | 1.765 | 5.593 | 8.509 | â |
| Cantat-Gaudin & Anders | 2020 | 313.621 | 47.4 | 1.765 | 5.593 | 8.509 | â |
| Liu & Pang | 2019 | 313.637 | 47.413 | 1.775 | 5.571 | 8.508 | â |
| Soubiran et al. | 2018 | 313.621 | 47.4 | â | â | â | -12.46 |
| Cantat-Gaudin et al. | 2018 | 313.621 | 47.4 | 1.765 | 5.593 | 8.509 | â |
| Loktin & Popova | 2017 | 313.725 | 47.417 | â | -0.272 | -0.157 | -21.77 |
| Dias et al. | 2014 | 313.725 | 47.417 | â | -1.5 | 1.94 | â |
| Gozha et al. | 2012 | 313.725 | 47.417 | â | â | â | â |
| Piskunov et al. | 2008 | 313.634 | 47.445 | â | â | â | â |
| Kharchenko et al. | 2007 | 313.72 | 47.42 | â | 0.42 | â | -6.0 |
| Piskunov et al. | 2007 | 313.634 | 47.445 | â | â | â | â |
| Kharchenko et al. | 2005 | 313.63 | 47.45 | â | 7.0 | 9.26 | -6.0 |
đĄ 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 | 99999â | 0.565 | 0.305 | 0.75 | 1429 | -0.037 | 373 | 0.61 | â |
| Li et al. | 2025 | 0.58 | 0.39 | â | 1331 | 0.053 | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.180(5) | â | â | â |
| Wei et al. | 2025 | 0.49 | 0.23 | â | 2090 | 0.000 | 795 | 0.63 | â |
| Almeida et al. | 2025 | 0.56 | 0.49 | â | 1429 | â | 373 | â | â |
| Alfonso et al. | 2024 | 0.58 | 0.20 | â | 1780 | -0.075 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 307(1) | â | â |
| Cavallo et al. | 2024 | 0.56 | 0.60 | â | 1259 | 0.120 | â | â | â |
| Hunt & Reffert | 2023 | 0.53 | 0.29 | 0.75 | 989 | â | â | â | â |
| Almeida et al. | 2023 | 0.55 | 0.32 | â | 1435 | 0.070 | 672(1) | 0.59 | â |
| He et al. | 2022 | â | 0.65 | â | 891 | â | â | â | â |
| Tarricq et al. | 2022 | 0.57 | â | â | 1622 | â | â | â | â |
| Dias et al. | 2021 | 0.56 | 0.49 | â | 1429 | -0.077 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.58 | 0.20 | â | 1549 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.56 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 1950 | -0.500 | â | â | â |
| Soubiran et al. | 2018 | 0.56 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 0.56 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 3.10 | 1.20 | â | 1514 | â | â | â | â |
| Gozha et al. | 2012 | 0.70 | â | â | 1288 | â | 214 | â | â |
| Piskunov et al. | 2008 | 0.70 | 0.00 | â | 1288 | â | 440(1) | â | â |
| Piskunov et al. | 2007 | 0.70 | 0.00 | â | 1288 | â | 148 | â | â |
| Kharchenko et al. | 2005 | 0.70 | 0.00 | â | 1288 | â | â | â | â |
(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.