King 25
(MWSC 3113; OCL 106; FSR 0127)
0.87
UTI
0.83
CN
1.0
Cdens
1.0
CC3
0.75
Clit
1.0
Cdup
Radius (P>50% members)
3.4 [arcmin]
- CN 0.83 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.75 Well-studied
- Cdup 1.0 Unique
Overview
King 25 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age and mass parameters (see Parameters). It is well-studied in the literature.
Relatively close
High extinction
Massive
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 291.127 | 13.698 | 0.315 | -1.381 | -3.962 | 21.385 |
| Almeida et al. | 2025 | 291.116 | 13.694 | â | â | â | â |
| Hunt & Reffert | 2024 | 291.134 | 13.697 | 0.313 | -1.387 | -3.95 | 37.877 |
| Cavallo et al. | 2024 | 291.13 | 13.691 | 0.314 | â | â | â |
| Hunt & Reffert | 2023 | 291.134 | 13.697 | 0.313 | -1.387 | -3.95 | 37.877 |
| Just et al. | 2023 | 291.119 | 13.698 | â | â | â | â |
| Dias et al. | 2021 | 291.116 | 13.694 | 0.313 | -1.373 | -3.961 | 13.25 |
| Cantat-Gaudin et al. | 2020 | 291.122 | 13.696 | 0.31 | -1.367 | -3.958 | â |
| Cantat-Gaudin & Anders | 2020 | 291.122 | 13.696 | 0.31 | -1.367 | -3.958 | â |
| Soubiran et al. | 2018 | 291.122 | 13.696 | â | â | â | 14.25 |
| Bica et al. | 2019 | 291.142 | 13.697 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 291.122 | 13.696 | 0.31 | -1.367 | -3.958 | â |
| Kharchenko et al. | 2016 | 291.119 | 13.698 | â | â | â | â |
| Kharchenko et al. | 2013 | 291.124 | 13.7 | â | 0.18 | -3.08 | 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 | 2.36 | 3.77 | â | 196 | â | 1172 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 5054* | â | â |
| Cavallo et al. | 2024 | 3.37 | 4.85 | â | 37 | 0.410 | â | â | â |
| Hunt & Reffert | 2023 | 2.83 | 5.02 | 1.89 | 83 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 282 | â | 259 | â | â |
| Dias et al. | 2021 | 2.36 | 3.77 | â | 196 | 0.430 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 3.09 | 4.17 | â | 45 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.95 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 2.95 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.95 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 1.80 | 4.13 | â | 282 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.80 | 4.13 | â | 282 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: invalid due to poor quality CMD. Isochrone match: worst fit.
Cavallo et al. (2024)
Gold sample.
Dias et al. (2002)
No cluster (Carraro, G.; Janes, K. A.; Eastman, J. D. 2005, MNRAS 364, 179)