Czernik 42
(MWSC 3650; OCL 245)
0.80
UTI
0.76
CN
1.0
Cdens
0.5
CC3
0.86
Clit
1.0
Cdup
Radius (P>50% members)
1.3 [arcmin]
- CN 0.76 Rich
- Cdens 1.0 Very dense
- CC3 0.5 Intermediate quality
- Clit 0.86 Well-studied
- Cdup 1.0 Unique
Overview
Czernik 42 is a rich, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age and mass parameters (see Parameters). It is well-studied in the literature.
Distant
High extinction
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | β | 339.895 | 59.91 | 0.206 | -3.412 | -2.546 | β |
| Almeida et al. | 2025 | 339.91 | 59.909 | β | β | β | β |
| Hunt & Reffert | 2024 | 339.893 | 59.908 | 0.203 | -3.409 | -2.545 | β |
| Cavallo et al. | 2024 | 339.901 | 59.909 | 0.204 | β | β | β |
| Hunt & Reffert | 2023 | 339.893 | 59.908 | 0.203 | -3.409 | -2.545 | β |
| Just et al. | 2023 | 339.897 | 59.915 | β | β | β | β |
| Dias et al. | 2021 | 339.91 | 59.909 | 0.168 | -3.364 | -2.522 | β |
| Cantat-Gaudin et al. | 2020 | 339.896 | 59.908 | 0.182 | -3.383 | -2.527 | β |
| SΓ‘nchez et al. | 2020 | 339.95 | 59.915 | β | -3.426 | -2.69 | β |
| Cantat-Gaudin & Anders | 2020 | 339.896 | 59.908 | 0.182 | -3.383 | -2.527 | β |
| Bica et al. | 2019 | 339.943 | 59.871 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 339.896 | 59.908 | 0.182 | -3.383 | -2.527 | β |
| Kharchenko et al. | 2016 | 339.897 | 59.915 | β | β | β | β |
| Dias et al. | 2014 | 339.95 | 59.915 | β | -2.41 | -1.56 | β |
| Kharchenko et al. | 2013 | 339.903 | 59.918 | β | -2.78 | -2.67 | β |
| Kharchenko et al. | 2012 | 339.903 | 59.918 | β | -2.78 | -2.67 | β |
| Dias et al. | 2002 | 339.95 | 59.915 | β | -2.41 | -1.56 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Almeida et al. | 2025 | 3.86 | 3.49 | β | 36 | β | 682 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 1697* | β | β |
| Cavallo et al. | 2024 | 4.72 | 3.60 | β | 282 | 0.700 | β | β | β |
| Hunt & Reffert | 2023 | 4.34 | 4.06 | 1.92 | 86 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 5 | β | 318 | β | β |
| Dias et al. | 2021 | 3.86 | 3.49 | β | 36 | -0.171 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 4.43 | 3.35 | β | 71 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 4.74 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 4.74 | β | β | β | β | β | β | β |
| Kharchenko et al. | 2016 | 4.00 | 3.79 | β | 5 | β | β | β | β |
| Kharchenko et al. | 2013 | 4.00 | 3.79 | β | 5 | β | β | β | β |
| Kharchenko et al. | 2012 | 4.00 | 3.79 | β | 5 | β | β | β | β |
| Dias et al. | 2002 | 2.58 | 5.39 | β | 10 | β | β | β | β |
(*): 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.