CWNU 1714
0.52
UTI
0.35
CN
0.89
Cdens
0.75
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members)
1.6 [arcmin]
- CN 0.35 Poorly populated
- Cdens 0.89 Dense
- CC3 0.75 High quality
- Clit 0.31 Poorly studied
- Cdup 1.0 Unique
Overview
CWNU 1714 is a poorly populated, dense object of high C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Very distant
Moderate extinction
Massive
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 100.59 | -1.515 | 0.166 | -0.12 | 0.544 | â |
| Hu & Soubiran | 2025 | 100.584 | -1.52 | â | â | â | â |
| Hunt & Reffert | 2024 | 100.595 | -1.515 | 0.169 | -0.121 | 0.548 | 87.248 |
| Cavallo et al. | 2024 | 100.584 | -1.52 | 0.164 | â | â | â |
| Hunt & Reffert | 2023 | 100.595 | -1.515 | 0.169 | -0.121 | 0.548 | 87.248 |
| He et al. | 2023 | 100.596 | -1.515 | 0.212 | -0.072 | 0.534 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Hu & Soubiran | 2025 | â | â | â | â | -0.300* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1278* | â | â |
| Cavallo et al. | 2024 | 3.96 | 1.53 | â | 631 | -0.140 | â | â | â |
| Hunt & Reffert | 2023 | 5.58 | 1.83 | 2.19 | 223 | â | â | â | â |
| He et al. | 2023 | 6.92 | 2.05 | â | 6 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Gold sample.