Czernik 40
(MWSC 3161; King 27; OCL 118)
0.82
UTI
0.75
CN
1.0
Cdens
0.75
CC3
0.79
Clit
1.0
Cdup
Radius (P>50% members)
1.5 [arcmin]
- CN 0.75 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.79 Well-studied
- Cdup 1.0 Unique
Overview
Czernik 40 is a rich, very dense object of high C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by high extinction. It is catalogued as a massive, 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
Massive
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 295.657 | 21.154 | 0.19 | -2.287 | -4.681 | 39.958 |
| Hunt & Reffert | 2024 | 295.662 | 21.155 | 0.199 | -2.308 | -4.708 | 42.822 |
| Celli et al. | 2024 | 295.661 | 21.145 | â | â | â | â |
| Cavallo et al. | 2024 | 295.67 | 21.151 | 0.199 | â | â | â |
| Hunt & Reffert | 2023 | 295.662 | 21.155 | 0.199 | -2.308 | -4.708 | 42.822 |
| Just et al. | 2023 | 295.651 | 21.14 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 295.661 | 21.145 | 0.207 | -2.249 | -4.613 | â |
| Cantat-Gaudin & Anders | 2020 | 295.661 | 21.145 | 0.207 | -2.249 | -4.613 | â |
| Bica et al. | 2019 | 295.661 | 21.152 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 295.661 | 21.145 | 0.207 | -2.249 | -4.613 | â |
| Loktin & Popova | 2017 | 295.665 | 21.166 | â | -2.344 | -10.698 | â |
| Kharchenko et al. | 2016 | 295.651 | 21.14 | â | â | â | â |
| Dias et al. | 2014 | 295.65 | 21.154 | â | -1.37 | -4.48 | â |
| Kharchenko et al. | 2013 | 295.657 | 21.143 | â | -0.87 | -10.1 | â |
| Dias et al. | 2002 | 295.65 | 21.154 | â | -1.37 | -4.48 | 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 | 3225* | â | â |
| Celli et al. | 2024 | â | â | â | 25 | â | 901 | â | â |
| Cavallo et al. | 2024 | 4.74 | 4.20 | â | 60 | 0.220 | â | â | â |
| Hunt & Reffert | 2023 | 4.70 | 4.35 | 2.23 | 46 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 851 | â | 2831 | â | â |
| Cantat-Gaudin et al. | 2020 | 4.61 | 3.43 | â | 25 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 4.24 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 4.24 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 2.64 | 1.90 | â | 977 | â | â | â | â |
| Kharchenko et al. | 2016 | 3.42 | 3.16 | â | 851 | â | â | â | â |
| Kharchenko et al. | 2013 | 3.42 | 3.16 | â | 851 | â | â | â | â |
| Dias et al. | 2002 | 3.09 | 3.07 | â | 794 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.