CWNU 2414
0.58
UTI
0.38
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members)
1.7 [arcmin]
- CN 0.38 Poorly populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.25 Poorly studied
- Cdup 1.0 Unique
Overview
CWNU 2414 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.
Distant
High 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 | 299.05 | 26.068 | 0.293 | -3.131 | -5.724 | 10.646 |
| Hunt & Reffert | 2024 | 299.047 | 26.069 | 0.297 | -3.135 | -5.708 | 24.715 |
| Cavallo et al. | 2024 | 299.1 | 26.087 | 0.297 | â | â | â |
| Hunt & Reffert | 2023 | 299.047 | 26.069 | 0.297 | -3.135 | -5.708 | 24.715 |
| He et al. | 2023 | 299.071 | 26.08 | 0.295 | -3.127 | -5.716 | 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 | 903* | â | â |
| Cavallo et al. | 2024 | 3.53 | 4.41 | â | 11 | 0.300 | â | â | â |
| Hunt & Reffert | 2023 | 3.17 | 4.32 | 2.46 | 11 | â | â | â | â |
| He et al. | 2023 | 3.31 | 5.05 | â | 16 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Gold sample.