Czernik 44
(MWSC 3740; OCL 265)
0.67
UTI
0.37
CN
1.0
Cdens
0.5
CC3
0.75
Clit
1.0
Cdup
Radius (P>50% members)
1.6 [arcmin]
- CN 0.37 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.5 Intermediate quality
- Clit 0.75 Well-studied
- Cdup 1.0 Unique
Overview
Czernik 44 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a large* distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is well-studied in the literature.
(*): The parallax distance estimate (~5.50 kpc) differs significantly from the median photometric distance (~3.82 kpc).
Distant
Moderate extinction
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 353.428 | 61.959 | 0.182 | -2.375 | -0.939 | â |
| Hunt & Reffert | 2024 | 353.433 | 61.955 | 0.187 | -2.303 | -0.859 | -95.544 |
| Cavallo et al. | 2024 | 353.646 | 61.922 | 0.185 | â | â | â |
| Hunt & Reffert | 2023 | 353.433 | 61.955 | 0.187 | -2.303 | -0.859 | -95.544 |
| Just et al. | 2023 | 353.388 | 61.935 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 353.415 | 61.954 | 0.184 | -2.377 | -0.878 | â |
| Cantat-Gaudin & Anders | 2020 | 353.415 | 61.954 | 0.184 | -2.377 | -0.878 | â |
| Bica et al. | 2019 | 353.387 | 61.94 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 353.415 | 61.954 | 0.184 | -2.377 | -0.878 | â |
| Loktin & Popova | 2017 | 353.4 | 61.95 | â | -1.811 | -2.844 | â |
| Kharchenko et al. | 2016 | 353.388 | 61.935 | â | â | â | â |
| Kharchenko et al. | 2013 | 353.395 | 61.938 | â | -3.76 | -2.19 | â |
| Kharchenko et al. | 2012 | 353.395 | 61.938 | â | -3.76 | -2.19 | â |
| Dias et al. | 2002 | 353.375 | 61.95 | â | 0.01 | -1.95 | â |
đĄ 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 |
|---|---|---|---|---|---|---|---|---|---|
| Hunt & Reffert | 2024 | â | â | â | â | â | 983* | â | â |
| Cavallo et al. | 2024 | 4.19 | 2.88 | â | 251 | 0.370 | â | â | â |
| Hunt & Reffert | 2023 | 4.77 | 3.17 | 2.17 | 88 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 32 | â | 20 | â | â |
| Cantat-Gaudin et al. | 2020 | 4.41 | 2.53 | â | 138 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 4.70 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 4.70 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 1.65 | 2.06 | â | 158 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.54 | 2.58 | â | 32 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.54 | 2.58 | â | 32 | â | â | â | â |
| Kharchenko et al. | 2012 | 1.54 | 2.58 | â | 32 | â | â | â | â |
| Dias et al. | 2002 | 3.45 | 4.59 | â | 158 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.