NGC 6704
(Collinder 390; MWSC 3007; OCL 82)
0.93
UTI
0.8
CN
1.0
Cdens
1.0
CC3
0.93
Clit
1.0
Cdup
Nm (P>50%)
232
Core radius and density
1.0 [pc], 19 [pc-2]
- CN 0.8 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.93 Very well-studied
- Cdup 1.0 Unique
Overview
NGC 6704 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age, metallicity, and mass parameters (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 | 99999β | 282.687 | -5.198 | 0.424 | -0.704 | -3.176 | 26.116 |
| Li et al. | 2025 | 282.687 | -5.203 | 0.434 | -0.73 | -3.139 | β |
| Yang et al. | 2025 | 282.688 | -5.199 | β | β | β | β |
| Almeida et al. | 2025 | 282.686 | -5.2 | β | β | β | β |
| Hunt & Reffert | 2024 | 282.688 | -5.199 | 0.415 | -0.706 | -3.202 | 28.505 |
| Cavallo et al. | 2024 | 282.689 | -5.194 | 0.415 | β | β | β |
| Hunt & Reffert | 2023 | 282.688 | -5.199 | 0.415 | -0.706 | -3.202 | 28.505 |
| Just et al. | 2023 | 282.679 | -5.212 | β | β | β | β |
| Dias et al. | 2022 | 282.689 | -5.2 | 0.419 | -0.693 | -3.203 | β |
| Jaehnig et al. | 2021 | 282.688 | -5.206 | 0.462 | -0.725 | -3.146 | β |
| Rain et al. | 2021 | 282.687 | -5.203 | 0.434 | -0.73 | -3.139 | β |
| Dias et al. | 2021 | 282.686 | -5.2 | 0.439 | -0.728 | -3.14 | β |
| Cantat-Gaudin et al. | 2020 | 282.687 | -5.203 | 0.434 | -0.73 | -3.139 | β |
| SΓ‘nchez et al. | 2020 | 282.688 | -5.205 | β | -0.714 | -3.009 | β |
| Cantat-Gaudin & Anders | 2020 | 282.687 | -5.203 | 0.434 | -0.73 | -3.139 | β |
| Bossini et al. | 2019 | 282.687 | -5.203 | β | β | β | β |
| Soubiran et al. | 2018 | 282.687 | -5.203 | β | β | β | 25.49 |
| Bica et al. | 2019 | 282.681 | -5.2 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 282.687 | -5.203 | 0.434 | -0.73 | -3.139 | β |
| Dias et al. | 2018 | β | β | β | 0.02 | -2.15 | β |
| Loktin & Popova | 2017 | 282.675 | -5.21 | β | 0.197 | -6.858 | β |
| Sampedro et al. | 2017 | 282.688 | -5.205 | β | -1.73 | -2.61 | β |
| Kharchenko et al. | 2016 | 282.679 | -5.212 | β | β | β | β |
| Dias et al. | 2014 | 282.688 | -5.205 | β | -1.69 | -2.04 | β |
| Kharchenko et al. | 2013 | 282.687 | -5.21 | β | -0.98 | -2.67 | β |
| Ahumada & Lapasset | 2007 | 282.7 | -5.2 | β | β | β | β |
| van den Bergh | 2006 | 282.725 | -5.2 | β | β | β | β |
| Dias et al. | 2002 | 282.688 | -5.205 | β | -1.69 | -2.04 | β |
| Lynga | 1987 | 282.703 | -5.201 | β | β | β | β |
| Sulentic et al. | 1973 | 282.708 | -5.203 | 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 | 2.16 | 2.45 | 1.46 | 119 | 0.157 | 730 | β | 0 |
| Li et al. | 2025 | 1.62 | 2.29 | β | 356 | 0.152 | β | β | β |
| Yang et al. | 2025 | β | β | β | 170 | 0.130(3) | β | β | β |
| Almeida et al. | 2025 | 1.76 | 2.45 | β | 121 | β | 730 | β | β |
| Hunt & Reffert | 2024 | 2.16 | 2.68 | 1.46 | 169 | β | 2225(1) | β | β |
| Cavallo et al. | 2024 | 2.39 | 2.83 | β | 117 | 0.660 | β | β | β |
| Hunt & Reffert | 2023 | 2.16 | 2.68 | 1.46 | 169 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 100 | β | 261 | β | β |
| Dias et al. | 2022 | 2.01(1) | 2.63(1) | β | 113(1) | 0.162(1) | β | β | β |
| Jaehnig et al. | 2021 | 2.14(1) | β | β | β | β | β | β | β |
| Rain et al. | 2021 | 2.16 | 2.27 | β | 170 | β | β | β | 0 |
| Dias et al. | 2021 | 1.76 | 2.45 | β | 121 | 0.273 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 2.04 | 2.23 | β | 200 | β | β | β | β |
| Kounkel et al. | 2020 | 2.32 | 2.88 | β | 191 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 2.16 | β | β | β | β | β | β | β |
| Bossini et al. | 2019 | 2.27 | 2.26 | β | 173 | 0.000 | β | β | β |
| Soubiran et al. | 2018 | 2.16 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 2.16 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 2.96 | 2.26 | β | 74 | β | β | β | β |
| Kharchenko et al. | 2016 | 2.18 | 3.02 | β | 100 | β | β | β | β |
| Kharchenko et al. | 2013 | 2.18 | 3.02 | β | 100 | β | β | β | β |
| Ahumada & Lapasset | 2007 | β | 2.27 | β | 72 | β | β | β | 0 |
| van den Bergh | 2006 | 2.97 | 2.27 | β | 72 | β | β | β | β |
| Dias et al. | 2002 | 2.97 | 2.26 | β | 73 | β | β | β | β |
| Lynga | 1987 | 1.81 | 3.22 | β | 20 | β | 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).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.99 (50th percentile).
Hu et al. (2021)
Ellipticities (core, all): e_core=0.0572, e_all=0.0254.
Rain et al. (2021)
This cluster was include in (Dias et al., 2002A&A...389..871D, Cat. B/ocl) however, parameters log(t)=8.237, Av=2.260, [Fe/H]=0.00 were taken from Bossini et al. (2019A&A...623A.108B, Cat. J/A+A/623/A108). The distance d=1775.0 (dmode+01) of Cantat-Gaudin et al. (2018A&A...618A..93C, Cat. J/A+A18/A93) was use to fit the isochrone.