Czernik 4
(MWSC 126)
0.21
UTI
0.25
CN
0.02
Cdens
0.12
CC3
0.32
Clit
1.0
Cdup
Nm (P>50%)
25
Core radius and density
2.3 [pc], 0.1 [pc-2]
- CN 0.25 Poorly populated
- Cdens 0.02 Very loose
- CC3 0.12 Very low quality
- Clit 0.32 Poorly studied
- Cdup 1.0 Unique
Overview
Czernik 4 is a poorly populated, very loose object of very low C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by high extinction. It is catalogued as a young cluster (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~3.16 kpc) differs significantly from the median photometric distance (~1.63 kpc).
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 23.886 | 61.493 | 0.316 | -2.289 | -0.352 | -49.201 |
| Just et al. | 2023 | 23.891 | 61.461 | â | â | â | â |
| Loktin & Popova | 2017 | 23.895 | 61.476 | â | 1.987 | -2.909 | -11.4 |
| Sampedro et al. | 2017 | 23.9 | 61.476 | â | -3.38 | -0.47 | â |
| Joshi et al. | 2016 | 23.902 | 61.463 | â | â | â | â |
| Kharchenko et al. | 2016 | 23.891 | 61.461 | â | â | â | â |
| Tadross | 2014 | 23.85 | 61.433 | â | â | â | â |
| Kharchenko et al. | 2013 | 23.902 | 61.463 | â | 1.84 | -1.84 | -11.4 |
| Kharchenko et al. | 2012 | 23.902 | 61.463 | â | 0.13 | -3.9 | â |
| Bukowiecki et al. | 2011 | 23.913 | 61.46 | â | â | â | â |
| Dias et al. | 2002 | 23.9 | 61.476 | â | 0.13 | -3.9 | -11.4 |
| Lynga | 1987 | 23.844 | 61.435 | â | â | â | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 1.63 | 3.15 | â | 52 | â | 202 | â | â |
| Just et al. | 2023 | â | â | â | 52 | â | 16 | â | â |
| Loktin & Popova | 2017 | 2.18 | 1.24 | â | 100 | â | â | â | â |
| Joshi et al. | 2016 | 1.63 | 3.15 | â | 52 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.63 | 3.15 | â | 52 | â | â | â | â |
| Tadross | 2014 | 1.63 | 3.34 | â | 100 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.63 | 3.15 | â | 52 | â | â | â | â |
| Bukowiecki et al. | 2012 | â | â | â | â | â | 389 | â | â |
| Kharchenko et al. | 2012 | 1.70 | 3.15 | â | 132 | â | â | â | â |
| Bukowiecki et al. | 2011 | 2.05(1) | 2.93 | â | 32 | â | â | â | â |
| Dias et al. | 2002 | 1.63 | 3.34 | â | 100 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA
