Czernik 29
(OCL 595; MWSC 1234)
0.64
UTI
0.47
CN
1.0
Cdens
0.5
CC3
0.62
Clit
1.0
Cdup
Stellar density (N50/rad)
11.1 [N/pc2]
- CN 0.47 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.5 Intermediate quality
- Clit 0.62 Moderately studied
- Cdup 1.0 Unique
Overview
Czernik 29 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is moderately studied in the literature.
Note: This object shares a moderate percentage of members with at least one entry reported in the same catalogue. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 112.106 | -15.4 | 0.24 | -1.553 | 1.322 | 88.409 |
| Hunt & Reffert | 2024 | 112.095 | -15.399 | 0.254 | -1.616 | 1.25 | 88.404 |
| Cavallo et al. | 2024 | 112.095 | -15.398 | 0.25 | â | â | â |
| Hunt & Reffert | 2023 | 112.095 | -15.399 | 0.254 | -1.616 | 1.25 | 88.404 |
| Cantat-Gaudin et al. | 2020 | 112.1 | -15.385 | 0.235 | -1.406 | 1.354 | â |
| Cantat-Gaudin & Anders | 2020 | 112.1 | -15.385 | 0.235 | -1.406 | 1.354 | â |
| Bica et al. | 2019 | 112.085 | -15.386 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 112.1 | -15.385 | 0.235 | -1.406 | 1.354 | â |
| Loktin & Popova | 2017 | 112.095 | -15.405 | â | -5.013 | 4.53 | â |
| Dias et al. | 2014 | 112.075 | -15.4 | â | -3.04 | 2.18 | â |
| van den Bergh | 2006 | 112.075 | -15.4 | â | â | â | â |
| Dias et al. | 2002 | 112.075 | -15.4 | â | -3.04 | 2.18 | 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 | 3.54 | 1.39 | 0.49 | 262 | -0.440 | 455 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 455(1) | â | â |
| Cavallo et al. | 2024 | 3.06 | 1.72 | â | 288 | -0.440 | â | â | â |
| Hunt & Reffert | 2023 | 3.57 | 1.32 | 0.49 | 243 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 3.48 | 1.09 | â | 151 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 3.80 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 3.80 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 3.51 | 0.81 | â | 617 | â | â | â | â |
| van den Bergh | 2006 | 4.17 | 1.49 | â | 200 | â | â | â | â |
| Dias et al. | 2002 | 3.00 | 1.46 | â | 282 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Gold sample.