Czernik 10
(MWSC 213)
0.74
UTI
0.46
CN
1.0
Cdens
0.75
CC3
0.75
Clit
1.0
Cdup
Radius (P>50% members)
1.0 [arcmin]
- CN 0.46 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.75 Well-studied
- Cdup 1.0 Unique
Overview
Czernik 10 is a poorly populated, 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 an intermediate-age cluster (see Parameters). It is well-studied in the literature.
Distant
High extinction
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | β | 38.479 | 60.171 | 0.251 | -1.13 | 0.403 | -68.704 |
| Hunt & Reffert | 2024 | 38.477 | 60.175 | 0.241 | -1.116 | 0.388 | -65.796 |
| Hunt & Reffert | 2023 | 38.477 | 60.175 | 0.241 | -1.116 | 0.388 | -65.796 |
| Just et al. | 2023 | 38.463 | 60.178 | β | β | β | β |
| Cantat-Gaudin et al. | 2020 | 38.483 | 60.167 | 0.239 | -1.178 | 0.267 | β |
| SΓ‘nchez et al. | 2020 | 38.475 | 60.167 | β | -1.125 | 0.087 | β |
| Cantat-Gaudin & Anders | 2020 | 38.483 | 60.167 | 0.239 | -1.178 | 0.267 | β |
| Soubiran et al. | 2018 | 38.483 | 60.167 | β | β | β | -68.36 |
| Cantat-Gaudin et al. | 2018 | 38.483 | 60.167 | 0.239 | -1.178 | 0.267 | β |
| Loktin & Popova | 2017 | 38.475 | 60.167 | β | -2.657 | -3.805 | β |
| Kharchenko et al. | 2016 | 38.463 | 60.178 | β | β | β | β |
| Dias et al. | 2014 | 38.475 | 60.167 | β | -0.55 | -2.23 | β |
| Kharchenko et al. | 2013 | 38.475 | 60.18 | β | -4.33 | -2.86 | β |
| Kharchenko et al. | 2012 | 38.475 | 60.18 | β | -4.33 | -2.86 | β |
π‘ 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 | β | β | β | β | β | 433* | β | β |
| Hunt & Reffert | 2023 | 3.87 | 4.57 | 1.41 | 130 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 318 | β | 89 | β | β |
| Cantat-Gaudin et al. | 2020 | 4.39 | 3.46 | β | 219 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 3.73 | β | β | β | β | β | β | β |
| Soubiran et al. | 2018 | 3.73 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 3.73 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 1.98 | 3.26 | β | 562 | β | β | β | β |
| Kharchenko et al. | 2016 | 2.50 | 4.18 | β | 318 | β | β | β | β |
| Kharchenko et al. | 2013 | 2.50 | 4.18 | β | 318 | β | β | β | β |
| Kharchenko et al. | 2012 | 2.50 | 4.18 | β | 318 | β | β | β | β |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
