NGC 6791
(Berkeley 46; MWSC 3088; OCL 142; FSR 0186; FoF 639)
1.0
UTI
1.0
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
N50 (P>50% members)
4657
Stellar density (N50/rad)
145.7 [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 6791 is a very rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, well above the mid-plane, affected by low extinction. It is catalogued as an extremely massive, near-solar metallicity, very 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 | 290.22 | 37.777 | 0.216 | -0.425 | -2.28 | -47.275 |
| Bijavara Seshashayana et al. | 2025 | 290.262 | 37.754 | β | β | β | β |
| Otto et al. | 2026 | 290.22 | 37.774 | β | -0.42 | -2.27 | -47.0 |
| Li et al. | 2025 | 290.221 | 37.778 | 0.192 | -0.421 | -2.269 | β |
| Guerco et al. | 2025 | 290.0 | 37.8 | 0.21 | -0.39 | -2.25 | -47.2 |
| Hu & Soubiran | 2025 | 290.221 | 37.777 | β | β | β | β |
| Carrasco-Varela et al. | 2025 | 290.375 | 37.778 | β | β | β | β |
| Almeida et al. | 2025 | 290.224 | 37.776 | β | β | β | β |
| Zhang et al. | 2024 | 290.22 | 37.774 | β | β | β | β |
| Hunt & Reffert | 2024 | 290.22 | 37.774 | 0.215 | -0.421 | -2.277 | -49.793 |
| Cavallo et al. | 2024 | 290.221 | 37.777 | 0.211 | β | β | β |
| Hunt & Reffert | 2023 | 290.22 | 37.774 | 0.215 | -0.421 | -2.277 | -49.793 |
| Angelo et al. | 2023 | 290.217 | 37.78 | β | -0.42 | -2.28 | β |
| Cordoni et al. | 2023 | 290.224 | 37.776 | 0.189 | -0.427 | -2.269 | β |
| Just et al. | 2023 | 290.216 | 37.778 | β | β | β | β |
| Jadhav & Subramaniam | 2021 | 290.221 | 37.778 | β | β | β | β |
| Jaehnig et al. | 2021 | 290.219 | 37.778 | 0.216 | -0.422 | -2.267 | β |
| Rain et al. | 2021 | 290.221 | 37.778 | 0.192 | -0.421 | -2.269 | β |
| Dias et al. | 2021 | 290.224 | 37.776 | 0.189 | -0.427 | -2.269 | -47.268 |
| Spina et al. | 2021 | 290.221 | 37.778 | 0.188 | -0.42 | -2.274 | β |
| Cantat-Gaudin et al. | 2020 | 290.221 | 37.778 | 0.192 | -0.421 | -2.269 | β |
| SΓ‘nchez et al. | 2020 | 290.221 | 37.772 | β | -0.412 | -2.225 | β |
| Donor et al. | 2020 | 290.22 | 37.78 | β | -0.44 | -2.25 | -46.9 |
| Zhong et al. | 2020 | 290.221 | 37.778 | β | -0.421 | -2.269 | -52.756 |
| Cantat-Gaudin & Anders | 2020 | 290.221 | 37.778 | 0.192 | -0.421 | -2.269 | β |
| Liu & Pang | 2019 | 290.226 | 37.779 | 0.266 | -0.452 | -2.275 | β |
| Bossini et al. | 2019 | 290.221 | 37.778 | β | β | β | β |
| Soubiran et al. | 2018 | 290.221 | 37.778 | β | β | β | -45.85 |
| Bica et al. | 2019 | 290.221 | 37.763 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 290.221 | 37.778 | 0.192 | -0.421 | -2.269 | β |
| Loktin & Popova | 2017 | 290.22 | 37.772 | β | -1.217 | -5.578 | -52.3 |
| Kharchenko et al. | 2016 | 290.216 | 37.778 | β | β | β | β |
| Dias et al. | 2014 | 290.221 | 37.772 | β | -0.83 | -4.91 | β |
| Kharchenko et al. | 2013 | 290.22 | 37.78 | β | -0.31 | -4.1 | -52.3 |
| Gozha et al. | 2012 | 290.221 | 37.772 | β | β | β | β |
| Bukowiecki et al. | 2011 | 290.225 | 37.774 | β | β | β | β |
| Kharchenko et al. | 2007 | 290.22 | 37.77 | β | 0.08 | β | β |
| Ahumada & Lapasset | 2007 | 290.225 | 37.767 | β | β | β | β |
| van den Bergh | 2006 | 290.221 | 37.772 | β | β | β | β |
| Chen et al. | 2003 | 290.231 | 37.791 | β | -3.17 | -7.74 | -57.0 |
| Dias et al. | 2002 | 290.221 | 37.772 | β | -0.83 | -4.91 | -47.4 |
| Lynga | 1987 | 290.185 | 37.842 | β | β | β | -68.0 |
| Sulentic et al. | 1973 | 290.194 | 37.848 | 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 | 4.48 | 0.41 | 0.36 | 6310 | 0.324 | 14253 | 0.25 | 35 |
| Bijavara Seshashayana et al. | 2025 | β | 0.70 | β | 8310 | 0.280(14) | β | β | β |
| Otto et al. | 2026 | β | β | β | 6310 | 0.300(15) | β | β | β |
| Li et al. | 2025 | 4.24 | 0.46 | β | 8138 | 0.327 | β | β | β |
| Guerco et al. | 2025 | β | β | β | 6310 | 0.330 | β | β | β |
| Hu & Soubiran | 2025 | β | β | β | β | -0.040(5) | β | β | β |
| Carrasco-Varela et al. | 2025 | 4.45 | 0.39 | β | 7228 | 0.500 | β | β | 35(1) |
| Almeida et al. | 2025 | 4.45 | 0.31 | β | 7228 | β | 24429 | β | β |
| Zhang et al. | 2024 | β | β | β | β | 0.233(1) | β | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 19407(1) | β | β |
| Cavallo et al. | 2024 | 3.44 | 0.98 | β | 9550 | -0.400 | β | β | β |
| Hunt & Reffert | 2023 | 4.22 | 0.65 | 0.36 | 3802 | β | β | β | β |
| Angelo et al. | 2023 | 4.15 | 0.41 | β | 7943 | 0.410 | 86(1) | β | β |
| Cordoni et al. | 2023 | 4.45 | 0.31 | β | 7228 | 0.399 | 5037 | 0.25 | 35(1) |
| Just et al. | 2023 | β | β | β | 4416 | β | 9099 | β | β |
| Spina et al. | 2022 | β | β | β | β | 0.350 | β | β | β |
| Jadhav & Subramaniam | 2021 | 4.23 | 0.70 | β | 6310 | β | 54394 | β | 24(1) |
| Jaehnig et al. | 2021 | 4.51(1) | β | β | β | β | β | β | β |
| Rain et al. | 2021 | 4.53 | 0.50 | β | 8318 | β | β | β | 48 |
| Dias et al. | 2021 | 4.45 | 0.31 | β | 7228 | 0.399 | β | β | β |
| Spina et al. | 2021 | 4.41 | β | β | 6310 | 0.332(20) | β | β | β |
| Cantat-Gaudin et al. | 2020 | 4.23 | 0.70 | β | 6310 | β | β | β | β |
| Kounkel et al. | 2020 | 4.06 | 0.74 | β | 2399 | β | β | β | β |
| Donor et al. | 2020 | β | β | β | β | 0.350 | β | β | β |
| Zhong et al. | 2020 | 4.53(1) | 0.31 | β | 9927 | 0.249 | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 4.53 | β | β | β | β | β | β | β |
| Liu & Pang | 2019 | β | β | β | 1950 | 0.250 | β | β | β |
| Bossini et al. | 2019 | 4.14 | 0.30 | β | 8453 | 0.400 | β | β | β |
| Soubiran et al. | 2018 | 4.53 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 4.53 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 5.47 | 0.41 | β | 4560 | β | β | β | β |
| Kharchenko et al. | 2016 | 4.93 | 0.37 | β | 4416 | β | β | β | β |
| Kharchenko et al. | 2013 | 4.93 | 0.37 | β | 4416 | 0.320 | β | β | β |
| Gozha et al. | 2012 | 5.85 | β | β | 4395 | 0.320 | β | β | β |
| Bukowiecki et al. | 2011 | 4.06(1) | 0.66 | β | 3548 | β | β | β | β |
| Ahumada & Lapasset | 2007 | β | 0.38 | β | 4365 | β | β | β | 75 |
| van den Bergh | 2006 | 5.85 | 0.38 | β | 4365 | β | β | β | β |
| Chen et al. | 2003 | 5.85 | 0.37 | β | 4390 | 0.150(1) | β | β | β |
| Dias et al. | 2002 | 5.04 | 0.50 | β | 8318 | 0.420 | β | β | β |
| Lynga | 1987 | 5.20 | 0.66 | β | 7079 | 0.040 | 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: intermediate fit. Silver sample.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.86 (50th percentile).
Rain et al. (2021)
The red limit of the straggler area is BP-RP=1.20.
Ahumada & Lapasset (2007)
The red limit of the straggler area is (B-V)=0.8. According to (1965ApJ...142..655K), stars 96, 63, and 106 are probable cluster members. Stars 63 and 106 are cited as blue stragglers in (1988PASP..100..338G). In (1965ApJ...142..655K) attention is drawn to several `red stragglers' that are probable cluster members. The CCD study (1990MNRAS.243..492K) mentions the existence of a possible FK Comae star. Spectra from (1965ApJ...142..655K): star 39, G0V; star 45, F2IV; star 102, F2IV; star 67, G2V; star 129, F9V; star 63, G0V. Star 123 = V6 (1993MNRAS.265...34K) is an EW variable (1993MNRAS.265...34K); the authors also discover two EW variables (V1 and V7) that they mark as stragglers: both stars have mean (B-V) colours redder than our limit of 0.8.