Czernik 23
(FSR 0834; MWSC 677; OCL 458)
0.90
UTI
0.77
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
26.2 [N/pc2]
- CN 0.77 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Czernik 23 is a rich, 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, intermediate-age cluster (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 | 87.525 | 28.898 | 0.261 | 0.007 | -1.78 | 17.589 |
| Almeida et al. | 2025 | 87.514 | 28.896 | β | β | β | β |
| Zhang et al. | 2024 | 87.528 | 28.898 | β | β | β | β |
| Hunt & Reffert | 2024 | 87.528 | 28.898 | 0.269 | 0.019 | -1.796 | 20.937 |
| Cavallo et al. | 2024 | 87.513 | 28.905 | 0.27 | β | β | β |
| Hunt & Reffert | 2023 | 87.528 | 28.898 | 0.269 | 0.019 | -1.796 | 20.937 |
| Almeida et al. | 2023 | 87.513 | 28.895 | β | β | β | β |
| Just et al. | 2023 | 87.516 | 28.901 | β | β | β | β |
| Dias et al. | 2021 | 87.514 | 28.896 | 0.246 | 0.053 | -1.78 | 14.314 |
| Cantat-Gaudin et al. | 2020 | 87.525 | 28.898 | 0.288 | 0.08 | -1.794 | β |
| SΓ‘nchez et al. | 2020 | 87.517 | 28.895 | β | -0.164 | -1.896 | β |
| Donor et al. | 2020 | 87.525 | 28.9 | β | 0.07 | -1.84 | 18.0 |
| Cantat-Gaudin & Anders | 2020 | 87.525 | 28.898 | 0.288 | 0.08 | -1.794 | β |
| Soubiran et al. | 2018 | 87.525 | 28.898 | β | β | β | 13.09 |
| Bica et al. | 2019 | 87.532 | 28.889 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 87.525 | 28.898 | 0.288 | 0.08 | -1.794 | β |
| Kharchenko et al. | 2016 | 87.516 | 28.901 | β | β | β | β |
| Dias et al. | 2014 | 87.517 | 28.895 | β | -0.02 | -0.32 | β |
| Kharchenko et al. | 2013 | 87.525 | 28.9 | β | -2.11 | -2.32 | β |
| Glushkova et al. | 2010 | 87.515 | 28.895 | β | β | β | β |
| Froebrich et al. | 2007 | 87.529 | 28.891 | β | β | β | β |
| Dias et al. | 2002 | 87.517 | 28.895 | β | -0.02 | -0.32 | 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 | 3.1 | 1.58 | 1.46 | 302 | -0.192 | 540 | 0.67 | β |
| Almeida et al. | 2025 | 3.10 | 1.74 | β | 313 | β | 514 | β | β |
| Zhang et al. | 2024 | β | β | β | β | -0.068(1) | β | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 1147(1) | β | β |
| Cavallo et al. | 2024 | 2.30 | 1.54 | β | 447 | -0.320 | β | β | β |
| Hunt & Reffert | 2023 | 3.04 | 1.32 | 1.46 | 431 | β | β | β | β |
| Almeida et al. | 2023 | 3.23 | 1.79 | β | 303 | -0.192 | 565(1) | 0.67 | β |
| Just et al. | 2023 | β | β | β | 302 | β | 346 | β | β |
| Dias et al. | 2021 | 3.10 | 1.74 | β | 313 | -0.132 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 3.96 | 1.49 | β | 269 | β | β | β | β |
| Donor et al. | 2020 | β | β | β | β | -0.280 | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 3.16 | β | β | β | β | β | β | β |
| Soubiran et al. | 2018 | 3.16 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 3.16 | β | β | β | β | β | β | β |
| Kharchenko et al. | 2016 | 2.45 | 1.62 | β | 302 | β | β | β | β |
| Kharchenko et al. | 2013 | 2.45 | 1.62 | β | 302 | β | β | β | β |
| Glushkova et al. | 2010 | 2.50 | 1.18 | β | 282 | β | β | β | β |
| Dias et al. | 2002 | 2.50 | 1.18 | β | 282 | 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.