Czernik 9
(MWSC 212)
0.90
UTI
0.75
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
24.9 [N/pc2]
- CN 0.75 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Czernik 9 is a rich, very dense object of high 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 metallicity and mass parameters (see Parameters). It is very well-studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 38.394 | 59.884 | 0.316 | -0.953 | 0.246 | -47.413 |
| Almeida et al. | 2025 | 38.398 | 59.882 | â | â | â | â |
| Hunt & Reffert | 2024 | 38.394 | 59.882 | 0.317 | -0.935 | 0.23 | -53.212 |
| Cavallo et al. | 2024 | 38.394 | 59.89 | 0.318 | â | â | â |
| Hunt & Reffert | 2023 | 38.394 | 59.882 | 0.317 | -0.935 | 0.23 | -53.212 |
| Almeida et al. | 2023 | 38.399 | 59.877 | â | â | â | â |
| Just et al. | 2023 | 38.373 | 59.872 | â | â | â | â |
| Dias et al. | 2021 | 38.398 | 59.882 | 0.303 | -0.919 | 0.256 | -46.83 |
| Cantat-Gaudin et al. | 2020 | 38.393 | 59.883 | 0.3 | -0.912 | 0.272 | â |
| Cantat-Gaudin & Anders | 2020 | 38.393 | 59.883 | 0.3 | -0.912 | 0.272 | â |
| Soubiran et al. | 2018 | 38.393 | 59.883 | â | â | â | -46.74 |
| Cantat-Gaudin et al. | 2018 | 38.393 | 59.883 | 0.3 | -0.912 | 0.272 | â |
| Loktin & Popova | 2017 | 38.385 | 59.887 | â | -1.62 | -2.696 | â |
| Kharchenko et al. | 2016 | 38.373 | 59.872 | â | â | â | â |
| Dias et al. | 2014 | 38.383 | 59.887 | â | -1.4 | 0.28 | â |
| Kharchenko et al. | 2013 | 38.385 | 59.875 | â | -2.62 | -3.09 | â |
| Kharchenko et al. | 2012 | 38.385 | 59.875 | â | -2.62 | -3.09 | â |
| Bukowiecki et al. | 2011 | 38.383 | 59.885 | â | â | â | â |
| Dias et al. | 2002 | 38.383 | 59.887 | â | -1.4 | 0.28 | 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 | 2.56 | 3.25 | 1.72 | 427 | -0.076 | 587 | 0.71 | â |
| Almeida et al. | 2025 | 2.56 | 3.20 | â | 395 | â | 587 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 725(1) | â | â |
| Cavallo et al. | 2024 | 3.84 | 3.70 | â | 191 | 0.520 | â | â | â |
| Hunt & Reffert | 2023 | 2.80 | 3.69 | 1.72 | 216 | â | â | â | â |
| Almeida et al. | 2023 | 2.51 | 3.28 | â | 347 | -0.146 | 489(1) | 0.71 | â |
| Just et al. | 2023 | â | â | â | 562 | â | 55 | â | â |
| Dias et al. | 2021 | 2.56 | 3.20 | â | 395 | -0.076 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 3.31 | 3.01 | â | 240 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 3.03 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 3.03 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 3.03 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 1.54 | 2.81 | â | 427 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.90 | 3.25 | â | 562 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.90 | 3.25 | â | 562 | â | â | â | â |
| Bukowiecki et al. | 2012 | â | â | â | â | â | 657 | â | â |
| Kharchenko et al. | 2012 | 1.90 | 3.25 | â | 562 | â | â | â | â |
| Bukowiecki et al. | 2011 | 3.08(1) | 2.88 | â | 447 | â | â | â | â |
| Dias et al. | 2002 | 1.66 | 3.26 | â | 631 | 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.
Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: intermediate fit. Silver sample.