CWNU 1042
0.46
UTI
0.38
CN
0.66
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members)
10.0 [arcmin]
- CN 0.38 Poorly populated
- Cdens 0.66 Moderately dense
- CC3 0.75 High quality
- Clit 0.25 Poorly studied
- Cdup 1.0 Unique
Overview
CWNU 1042 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is poorly studied in the literature.
Relatively close
Moderate extinction
Near-solar metallicity
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 58.418 | 53.214 | 0.858 | -0.428 | -1.472 | 1.522 |
| Hunt & Reffert | 2024 | 58.462 | 53.207 | 0.851 | -0.445 | -1.491 | 1.686 |
| Cavallo et al. | 2024 | 58.306 | 53.205 | 0.843 | â | â | â |
| Hunt & Reffert | 2023 | 58.462 | 53.207 | 0.851 | -0.445 | -1.491 | 1.686 |
| He et al. | 2022 | 58.503 | 53.206 | 0.862 | -0.347 | -1.451 | 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 | 162* | â | â |
| Cavallo et al. | 2024 | 1.24 | 2.66 | â | 6 | -0.210 | â | â | â |
| Hunt & Reffert | 2023 | 1.12 | 3.17 | 1.97 | 6 | â | â | â | â |
| He et al. | 2022 | â | 3.00 | â | 4 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Silver sample.