CWNU 1702
0.45
UTI
0.0
CN
0.77
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad)
3.9 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.77 Dense
- CC3 1.0 Very high quality
- Clit 0.25 Poorly studied
- Cdup 1.0 Unique
Overview
CWNU 1702 is a sparse, dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by very high extinction. It is catalogued as a massive, near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 258.416 | -38.872 | 0.257 | -1.061 | -2.637 | 5.578 |
| Hunt & Reffert | 2024 | 258.397 | -38.868 | 0.254 | -1.058 | -2.665 | -53.16 |
| Cavallo et al. | 2024 | 258.428 | -38.888 | 0.254 | â | â | â |
| Hunt & Reffert | 2023 | 258.397 | -38.868 | 0.254 | -1.058 | -2.665 | -53.16 |
| He et al. | 2023 | 258.43 | -38.872 | 0.259 | -1.038 | -2.628 | 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 | 3.73 | 5.48 | 2.43 | 4 | 0.210 | 2618 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 2618(1) | â | â |
| Cavallo et al. | 2024 | 3.73 | 5.33 | â | 4 | 0.210 | â | â | â |
| Hunt & Reffert | 2023 | 3.68 | 5.48 | 2.43 | 13 | â | â | â | â |
| He et al. | 2023 | 4.47 | 6.80 | â | 4 | 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)
Silver sample.