NGC 659
(MWSC 138)
0.96
UTI
0.8
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
3.1 [arcmin]
- CN 0.8 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
NGC 659 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 massive, near-solar metallicity, young 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.
Relatively close
Moderate extinction
Massive
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 26.097 | 60.678 | 0.301 | -0.833 | -0.299 | -41.518 |
| Almeida et al. | 2025 | 26.103 | 60.677 | â | â | â | â |
| Hunt & Reffert | 2024 | 26.086 | 60.672 | 0.301 | -0.838 | -0.324 | -48.222 |
| Celli et al. | 2024 | 26.108 | 60.679 | â | â | â | â |
| Cavallo et al. | 2024 | 26.093 | 60.675 | 0.302 | â | â | â |
| Hunt & Reffert | 2023 | 26.086 | 60.672 | 0.301 | -0.838 | -0.324 | -48.222 |
| Almeida et al. | 2023 | 26.102 | 60.671 | â | â | â | â |
| Just et al. | 2023 | 26.082 | 60.667 | â | â | â | â |
| Jaehnig et al. | 2021 | 26.104 | 60.679 | 0.318 | -0.802 | -0.261 | â |
| Rain et al. | 2021 | 26.108 | 60.679 | 0.287 | -0.796 | -0.257 | â |
| Dias et al. | 2021 | 26.103 | 60.677 | 0.286 | -0.792 | -0.26 | -57.228 |
| Cantat-Gaudin et al. | 2020 | 26.108 | 60.679 | 0.287 | -0.796 | -0.257 | â |
| Cantat-Gaudin & Anders | 2020 | 26.108 | 60.679 | 0.287 | -0.796 | -0.257 | â |
| Dias et al. | 2019 | 26.1 | 60.673 | 0.272 | -0.799 | -0.276 | 77.81 |
| Cantat-Gaudin et al. | 2018 | 26.108 | 60.679 | 0.287 | -0.796 | -0.257 | â |
| Loktin & Popova | 2017 | 26.1 | 60.673 | â | 0.042 | -0.103 | â |
| Kharchenko et al. | 2016 | 26.082 | 60.667 | â | â | â | â |
| Dias et al. | 2014 | 26.1 | 60.673 | â | -1.43 | -0.31 | â |
| Kharchenko et al. | 2013 | 26.092 | 60.67 | â | -0.46 | -0.63 | â |
| Kharchenko et al. | 2012 | 26.092 | 60.67 | â | -0.46 | -0.63 | â |
| Piskunov et al. | 2008 | 26.087 | 60.669 | â | â | â | â |
| van den Bergh | 2006 | 26.1 | 60.667 | â | â | â | â |
| Kharchenko et al. | 2005 | 26.1 | 60.67 | â | -2.97 | -0.55 | â |
| Dias et al. | 2002 | 26.1 | 60.673 | â | -2.67 | 1.07 | â |
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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Almeida et al. | 2025 | 2.60 | 2.16 | â | 22 | â | 558 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1892* | â | â |
| Celli et al. | 2024 | â | â | â | 16 | â | 1487 | â | â |
| Cavallo et al. | 2024 | 3.28 | 2.10 | â | 41 | 0.600 | â | â | â |
| Hunt & Reffert | 2023 | 2.92 | 2.12 | 1.58 | 42 | â | â | â | â |
| Almeida et al. | 2023 | 2.63 | 2.17 | â | 24 | -0.083 | 1094* | 0.54 | â |
| Just et al. | 2023 | â | â | â | 58 | â | 290 | â | â |
| Jaehnig et al. | 2021 | 3.13* | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 3.17 | 2.02 | â | 35 | â | â | â | 0 |
| Dias et al. | 2021 | 2.60 | 2.16 | â | 22 | -0.046 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 3.31 | 1.86 | â | 15 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 3.17 | â | â | â | â | â | â | â |
| Dias et al. | 2019 | 3.02 | 1.71 | â | 27 | -0.524 | â | â | â |
| Cantat-Gaudin et al. | 2018 | 3.17 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 1.98 | 2.00 | â | 36 | â | â | â | â |
| Kharchenko et al. | 2016 | 2.30 | 2.02 | â | 58 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.30 | 2.02 | â | 58 | â | â | â | â |
| Kharchenko et al. | 2012 | 2.30 | 2.02 | â | 58 | â | â | â | â |
| Piskunov et al. | 2008 | 1.94 | 2.02 | â | 63 | â | â | â | â |
| van den Bergh | 2006 | 1.94 | 2.02 | â | 35 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.94 | 2.02 | â | 63 | â | â | â | â |
| Dias et al. | 2002 | 1.94 | 2.02 | â | 35 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: intermediate fit. Silver sample.
Cavallo et al. (2024)
Gold sample.