CWNU 1295
0.26
UTI
0.44
CN
1.0
Cdens
0.75
CC3
0.35
Clit
0.46
Cdup
Stellar density (N50/rad)
7.0 [N/pc2]
- CN 0.44 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.35 Poorly studied
- Cdup 0.46 Possibly duplicate
Overview
CWNU 1295 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.
â ī¸ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 92.077 | 28.074 | 0.256 | -0.198 | -1.693 | 0.528 |
| Hu & Soubiran | 2025 | 92.068 | 28.063 | â | â | â | â |
| Zhang et al. | 2024 | 92.082 | 28.073 | â | â | â | â |
| Hunt & Reffert | 2024 | 92.082 | 28.073 | 0.256 | -0.216 | -1.668 | 7.407 |
| Cavallo et al. | 2024 | 92.068 | 28.063 | 0.256 | â | â | â |
| Hunt & Reffert | 2023 | 92.082 | 28.073 | 0.256 | -0.216 | -1.668 | 7.407 |
| He et al. | 2023 | 92.078 | 28.071 | 0.283 | -0.196 | -1.683 | 8.32 |
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 | 3.55 | 1.19 | 1.55 | 560 | -0.250 | 520 | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.250(5) | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.118(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 520(1) | â | â |
| Cavallo et al. | 2024 | 3.05 | 1.19 | â | 562 | -0.350 | â | â | â |
| Hunt & Reffert | 2023 | 3.55 | 0.86 | 1.55 | 560 | â | â | â | â |
| He et al. | 2023 | 3.98 | 1.30 | â | 282 | 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)
Gold sample.