Koposov 63
(FSR 0869; MWSC 772; Teutsch J0610.0+2434; MWSC 773)
0.88
UTI
0.64
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
2.4 [arcmin]
- CN 0.64 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Koposov 63 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, old cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is very well-studied in the literature.
Distant
Moderate extinction
Near-solar metallicity
Old
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | β | 92.5 | 24.571 | 0.222 | 0.526 | -0.428 | 36.548 |
| Li et al. | 2025 | 92.499 | 24.567 | 0.206 | 0.546 | -0.447 | β |
| Hu & Soubiran | 2025 | 92.509 | 24.562 | β | β | β | β |
| Zhang et al. | 2024 | 92.521 | 24.565 | β | β | β | β |
| Hunt & Reffert | 2024 | 92.521 | 24.565 | 0.225 | 0.513 | -0.443 | 25.168 |
| Cavallo et al. | 2024 | 92.509 | 24.563 | 0.227 | β | β | β |
| Hunt & Reffert | 2023 | 92.521 | 24.565 | 0.225 | 0.513 | -0.443 | 25.168 |
| Just et al. | 2023 | 92.499 | 24.551 | β | β | β | β |
| Cantat-Gaudin et al. | 2020 | 92.499 | 24.567 | 0.206 | 0.546 | -0.447 | β |
| SΓ‘nchez et al. | 2020 | 92.508 | 24.561 | β | 0.564 | -0.514 | β |
| Cantat-Gaudin & Anders | 2020 | 92.499 | 24.567 | 0.206 | 0.546 | -0.447 | β |
| Monteiro & Dias | 2019 | 92.521 | 24.559 | β | 0.533 | -0.481 | 2.544 |
| Soubiran et al. | 2018 | 92.499 | 24.567 | β | β | β | 13.68 |
| Bica et al. | 2019 | 92.528 | 24.555 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 92.499 | 24.567 | 0.206 | 0.546 | -0.447 | β |
| Loktin & Popova | 2017 | 92.505 | 24.562 | β | 0.548 | -0.704 | β |
| Kharchenko et al. | 2016 | 92.499 | 24.551 | β | β | β | β |
| Dias et al. | 2014 | 92.508 | 24.561 | β | 0.31 | -1.4 | β |
| Kharchenko et al. | 2013 | 92.508 | 24.55 | β | 1.65 | -2.1 | β |
| Glushkova et al. | 2010 | 92.507 | 24.561 | β | β | β | β |
| Koposov et al. | 2008 | 92.506 | 24.561 | β | β | β | β |
| Froebrich et al. | 2007 | 92.521 | 24.559 | β | β | β | β |
| Dias et al. | 2002 | 92.508 | 24.561 | β | 0.31 | -1.4 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 3.63 | 1.80 | β | 1198 | -0.542 | β | β | β |
| Hu & Soubiran | 2025 | β | β | β | β | -0.220* | β | β | β |
| Zhang et al. | 2024 | β | β | β | β | -0.260* | β | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 821* | β | β |
| Cavallo et al. | 2024 | 3.18 | 1.18 | β | 1288 | 0.340 | β | β | β |
| Hunt & Reffert | 2023 | 4.13 | 1.58 | 2.06 | 601 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 1660 | β | 95 | β | β |
| Cantat-Gaudin et al. | 2020 | 3.78 | 1.06 | β | 1950 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 4.26 | β | β | β | β | β | β | β |
| Monteiro & Dias | 2019 | 4.63 | 1.26 | β | 839 | 0.034 | β | β | β |
| Soubiran et al. | 2018 | 4.26 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 4.26 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 4.56 | 1.20 | β | 200 | β | β | β | β |
| Kharchenko et al. | 2016 | 3.22 | 1.55 | β | 1660 | β | β | β | β |
| Kharchenko et al. | 2013 | 3.22 | 1.55 | β | 1660 | β | β | β | β |
| Glushkova et al. | 2010 | 3.00 | 0.81 | β | 1413 | β | β | β | β |
| Koposov et al. | 2008 | 3.00 | 0.81 | β | 1413 | β | β | β | β |
| Dias et al. | 2002 | 3.00 | 0.81 | β | 1413 | β | β | β | β |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.