Czernik 23
(FSR 0834; MWSC 677; OCL 458)
- 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
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | – | 87.525 | 28.898 | 0.261 | 0.007 | -1.78 | 17.589 |
| Almeida et al. | 2025 | 87.514 | 28.896 | – | – | – | – |
| Zhang et al. | 2024 | 87.528 | 28.898 | – | – | – | – |
| 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 | – | – | – |
| Hunt & Reffert | 2023 | 87.528 | 28.898 | 0.269 | 0.019 | -1.796 | 20.937 |
| Just et al. | 2023 | 87.516 | 28.901 | – | – | – | – |
| 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 | – |
| Donor et al. | 2020 | 87.525 | 28.9 | – | 0.07 | -1.84 | 18.0 |
| Soubiran et al. | 2018 | 87.525 | 28.898 | – | – | – | 13.09 |
| Bica et al. | 2019 | 87.532 | 28.889 | – | – | – | – |
| Cantat-Gaudin et al. | 2018 | 87.525 | 28.898 | 0.288 | 0.08 | -1.794 | – |
| Kharchenko et al. | 2016 | 87.516 | 28.901 | – | – | – | – |
| Kharchenko et al. | 2013 | 87.525 | 28.9 | – | -2.11 | -2.32 | – |
| Glushkova et al. | 2010 | 87.515 | 28.895 | – | – | – | – |
| Froebrich et al. | 2007 | 87.529 | 28.891 | – | – | – | – |
| Dias et al. | 2002 | 87.517 | 28.895 | – | -0.02 | -0.32 | – |
💡 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 | 3.10 | 1.74 | – | 313 | – | 514 | – | – |
| Zhang et al. | 2024 | – | – | – | – | -0.068* | – | – | – |
| Hunt & Reffert | 2024 | – | – | – | – | – | 1147* | – | – |
| Cavallo et al. | 2024 | 2.30 | 1.54 | – | 447 | -0.320 | – | – | – |
| Hunt & Reffert | 2023 | 3.04 | 1.32 | 1.46 | 431 | – | – | – | – |
| Just et al. | 2023 | – | – | – | 302 | – | 346 | – | – |
| Dias et al. | 2021 | 3.10 | 1.74 | – | 313 | -0.132 | – | – | – |
| Cantat-Gaudin et al. | 2020 | 3.96 | 1.49 | – | 269 | – | – | – | – |
| Donor et al. | 2020 | – | – | – | – | -0.280 | – | – | – |
| Soubiran et al. | 2018 | 3.16 | – | – | – | – | – | – | – |
| Cantat-Gaudin et al. | 2018 | 3.16 | – | – | – | – | – | – | – |
| Kharchenko et al. | 2016 | 2.45 | 1.62 | – | 302 | – | – | – | – |
| Kharchenko et al. | 2013 | 2.45 | 1.62 | – | 302 | – | – | – | – |
| Glushkova et al. | 2010 | 2.50 | 1.18 | – | 282 | – | – | – | – |
| Dias et al. | 2002 | 2.50 | 1.18 | – | 282 | – | – | – | – |
💡 Note: The parameters are sometimes
transformed from their original values to match the format of the
columns shown here, see FAQ.
The columns DAv, Bfr, BSS correspond to differential
extinction, binary fraction, and blue stragglers, respectively.
BSS values can be listed as fractions or integers.
(*): indicates that this parameter is
assigned more than one value in the corresponding reference.
Almeida et al. (2025): Mass determination: good fit. Isochrone match: good fit. Gold sample.
Cavallo et al. (2024): Gold sample.