CWNU 1281
0.33
UTI
0.35
CN
0.22
Cdens
0.5
CC3
0.3
Clit
1.0
Cdup
Stellar density (N50/rad)
1.1 [N/pc2]
- CN 0.35 Poorly populated
- Cdens 0.22 Very loose
- CC3 0.5 Intermediate quality
- Clit 0.3 Poorly studied
- Cdup 1.0 Unique
Overview
CWNU 1281 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.
Note: This object shares a very small percentage of members with a later 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 | 100.676 | 4.726 | 0.643 | -1.964 | 0.794 | â |
| Zhang et al. | 2024 | 100.645 | 4.728 | â | â | â | â |
| Hunt & Reffert | 2024 | 100.645 | 4.728 | 0.641 | -1.959 | 0.798 | â |
| Cavallo et al. | 2024 | 100.633 | 4.7 | 0.639 | â | â | â |
| Hunt & Reffert | 2023 | 100.645 | 4.728 | 0.641 | -1.959 | 0.798 | â |
| He et al. | 2023 | 100.62 | 4.753 | 0.644 | -1.972 | 0.816 | 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 | 1.48 | 0.95 | 0.87 | 58 | 0.051 | 170 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.089(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 170(1) | â | â |
| Cavallo et al. | 2024 | 1.51 | 0.95 | â | 58 | 0.190 | â | â | â |
| Hunt & Reffert | 2023 | 1.47 | 0.91 | 0.87 | 69 | â | â | â | â |
| He et al. | 2023 | 1.48 | 1.10 | â | 40 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Palma et al. (2025)
Part of multiple system G40, along with HSC_1641, CWNU_158, HSC_1636 and Collinder_104.
Cavallo et al. (2024)
Gold sample.