Czernik 3
(MWSC 98)
0.77
UTI
0.77
CN
1.0
Cdens
0.38
CC3
0.86
Clit
1.0
Cdup
Radius (P>50% members)
1.7 [arcmin]
- CN 0.77 Rich
- Cdens 1.0 Very dense
- CC3 0.38 Low quality
- Clit 0.86 Well-studied
- Cdup 1.0 Unique
Overview
Czernik 3 is a rich, very dense object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the mass parameter (see Parameters). It is well-studied in the literature.
Distant
High extinction
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | β | 15.783 | 62.788 | 0.211 | -0.185 | -0.366 | -69.018 |
| Almeida et al. | 2025 | 15.765 | 62.79 | β | β | β | β |
| Hunt & Reffert | 2024 | 15.777 | 62.785 | 0.217 | -0.194 | -0.392 | -72.631 |
| Cavallo et al. | 2024 | 15.769 | 62.787 | 0.219 | β | β | β |
| Hunt & Reffert | 2023 | 15.777 | 62.785 | 0.217 | -0.194 | -0.392 | -72.631 |
| Just et al. | 2023 | 15.777 | 62.783 | β | β | β | β |
| Dias et al. | 2021 | 15.765 | 62.79 | 0.198 | -0.206 | -0.276 | β |
| Cantat-Gaudin et al. | 2020 | 15.78 | 62.787 | 0.195 | -0.22 | -0.296 | β |
| SΓ‘nchez et al. | 2020 | 15.775 | 62.783 | β | -0.044 | -0.789 | β |
| Cantat-Gaudin & Anders | 2020 | 15.78 | 62.787 | 0.195 | -0.22 | -0.296 | β |
| Cantat-Gaudin et al. | 2018 | 15.78 | 62.787 | 0.195 | -0.22 | -0.296 | β |
| Loktin & Popova | 2017 | 15.78 | 62.783 | β | -1.483 | -0.061 | β |
| Kharchenko et al. | 2016 | 15.777 | 62.783 | β | β | β | β |
| Dias et al. | 2014 | 15.775 | 62.783 | β | 0.69 | 5.2 | β |
| Kharchenko et al. | 2013 | 15.787 | 62.787 | β | -1.55 | 0.36 | β |
| Kharchenko et al. | 2012 | 15.787 | 62.787 | β | -1.55 | 0.36 | β |
| Dias et al. | 2002 | 15.775 | 62.783 | β | -1.55 | 0.36 | 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 | 4.50 | 3.29 | β | 318 | β | 450 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 792* | β | β |
| Cavallo et al. | 2024 | 3.82 | 3.16 | β | 437 | 0.540 | β | β | β |
| Hunt & Reffert | 2023 | 3.79 | 3.48 | 1.90 | 215 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 631 | β | 36 | β | β |
| Dias et al. | 2021 | 4.50 | 3.29 | β | 318 | -0.100 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 4.41 | 2.91 | β | 347 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 4.47 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 4.47 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 1.48 | 2.11 | β | 251 | β | β | β | β |
| Kharchenko et al. | 2016 | 1.60 | 3.10 | β | 631 | β | β | β | β |
| Kharchenko et al. | 2013 | 1.60 | 3.10 | β | 631 | β | β | β | β |
| Kharchenko et al. | 2012 | 1.60 | 3.10 | β | 631 | β | β | β | β |
| Dias et al. | 2002 | 1.41 | 4.40 | β | 100 | 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.