Czernik 19
(MWSC 441; OCL 443; FSR 0792)
0.91
UTI
0.78
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
12.3 [N/pc2]
- CN 0.78 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Czernik 19 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age and metallicity parameters (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 | 74.262 | 28.764 | 0.39 | 0.966 | -2.127 | 16.676 |
| Li et al. | 2025 | 74.258 | 28.763 | 0.367 | 1.049 | -2.126 | β |
| Almeida et al. | 2025 | 74.244 | 28.763 | β | β | β | β |
| Zhang et al. | 2024 | 74.274 | 28.77 | β | β | β | β |
| Hunt & Reffert | 2024 | 74.274 | 28.77 | 0.395 | 0.953 | -2.132 | 15.856 |
| Cavallo et al. | 2024 | 74.247 | 28.774 | 0.392 | β | β | β |
| Hunt & Reffert | 2023 | 74.274 | 28.77 | 0.395 | 0.953 | -2.132 | 15.856 |
| Almeida et al. | 2023 | 74.254 | 28.757 | β | β | β | β |
| Just et al. | 2023 | 74.268 | 28.781 | β | β | β | β |
| Dias et al. | 2021 | 74.244 | 28.763 | 0.368 | 1.062 | -2.143 | β |
| Cantat-Gaudin et al. | 2020 | 74.258 | 28.763 | 0.367 | 1.049 | -2.126 | β |
| SΓ‘nchez et al. | 2020 | 74.287 | 28.78 | β | 1.223 | -2.262 | β |
| Zhong et al. | 2020 | 74.258 | 28.763 | β | 1.049 | -2.126 | 23.102 |
| Cantat-Gaudin & Anders | 2020 | 74.258 | 28.763 | 0.367 | 1.049 | -2.126 | β |
| Bossini et al. | 2019 | 74.258 | 28.763 | β | β | β | β |
| Bica et al. | 2019 | 74.259 | 28.783 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 74.258 | 28.763 | 0.367 | 1.049 | -2.126 | β |
| Loktin & Popova | 2017 | 74.28 | 28.781 | β | 1.451 | -2.113 | β |
| Kharchenko et al. | 2016 | 74.268 | 28.781 | β | β | β | β |
| Dias et al. | 2014 | 74.287 | 28.78 | β | 4.39 | -1.93 | β |
| Kharchenko et al. | 2013 | 74.277 | 28.781 | β | 1.22 | -2.68 | β |
| Kharchenko et al. | 2012 | 74.277 | 28.781 | β | 1.22 | -2.68 | β |
| Bukowiecki et al. | 2011 | 74.258 | 28.792 | β | β | β | β |
| Dias et al. | 2002 | 74.287 | 28.78 | β | 4.39 | -1.93 | 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 | 2.5 | 2.08 | 0.58 | 80 | -0.133 | 623 | 0.66 | β |
| Li et al. | 2025 | 1.98 | 2.12 | β | 271 | -0.247 | β | β | β |
| Almeida et al. | 2025 | 2.07 | 2.19 | β | 66 | β | 502 | β | β |
| Zhang et al. | 2024 | β | β | β | β | -0.293(1) | β | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 1038(1) | β | β |
| Cavallo et al. | 2024 | 2.65 | 2.15 | β | 89 | 0.370 | β | β | β |
| Hunt & Reffert | 2023 | 2.30 | 1.86 | 0.58 | 142 | β | β | β | β |
| Almeida et al. | 2023 | 2.12 | 2.15 | β | 150 | -0.133 | 623(1) | 0.66 | β |
| Just et al. | 2023 | β | β | β | 68 | β | 483 | β | β |
| Dias et al. | 2021 | 2.07 | 2.19 | β | 66 | -0.160 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 2.58 | 1.78 | β | 204 | β | β | β | β |
| Zhong et al. | 2020 | 2.86 | 1.95 | β | 8003 | -0.106 | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 2.52 | β | β | β | β | β | β | β |
| Bossini et al. | 2019 | 2.86 | 1.95 | β | 101 | 0.000 | β | β | β |
| Cantat-Gaudin et al. | 2018 | 2.52 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 2.38 | 1.57 | β | 71 | β | β | β | β |
| Kharchenko et al. | 2016 | 2.50 | 2.08 | β | 68 | β | β | β | β |
| Kharchenko et al. | 2013 | 2.50 | 2.08 | β | 68 | β | β | β | β |
| Bukowiecki et al. | 2012 | β | β | β | β | β | 1242 | β | β |
| Kharchenko et al. | 2012 | 2.50 | 2.08 | β | 68 | β | β | β | β |
| Bukowiecki et al. | 2011 | 3.27(1) | 1.74 | β | 178 | β | β | β | β |
| Dias et al. | 2002 | 2.50 | 2.08 | β | 25 | β | β | β | β |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


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