CWNU 287
(OCSN 151)
0.62
UTI
0.52
CN
1.0
Cdens
0.75
CC3
0.4
Clit
1.0
Cdup
Stellar density (N50/rad)
10.8 [N/pc2]
- CN 0.52 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.4 Poorly studied
- Cdup 1.0 Unique
Overview
CWNU 287 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a metal-rich, young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is poorly studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 155.257 | -55.925 | 2.282 | -14.53 | 2.433 | 9.637 |
| Wei et al. | 2025 | 155.429 | -55.984 | 2.228 | -14.658 | 2.509 | â |
| Hunt & Reffert | 2024 | 155.3 | -55.972 | 2.284 | -14.537 | 2.438 | 14.469 |
| Cavallo et al. | 2024 | 155.284 | -55.894 | 2.286 | â | â | â |
| Hunt & Reffert | 2023 | 155.3 | -55.972 | 2.284 | -14.537 | 2.438 | 14.469 |
| Qin et al. | 2023 | 155.21 | -55.94 | 2.28 | -14.49 | 2.47 | 8.92 |
| He et al. | 2022 | 154.79 | -55.861 | 2.266 | -14.409 | 2.718 | â |
| He et al. | 2022 | 155.233 | -55.977 | 2.28 | -14.5 | 2.51 | 12.2 |
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 | 0.46 | 0.335 | 0.51 | 54 | 0.500 | 68 | 0.32 | â |
| Wei et al. | 2025 | 0.58 | 0.37 | â | 59 | 0.500 | 90 | 0.32 | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 45(1) | â | â |
| Cavallo et al. | 2024 | 0.42 | 0.77 | â | 132 | -0.190 | â | â | â |
| Hunt & Reffert | 2023 | 0.42 | 0.13 | 0.51 | 100 | â | â | â | â |
| Qin et al. | 2023 | 0.57 | 0.53 | â | 32 | â | â | â | â |
| He et al. | 2022 | â | 0.30 | â | 35 | â | â | â | â |
| He et al. | 2022 | 0.46 | 0.30 | â | 50 | 0.537 | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Palma et al. (2025)
Classified as optical pair P275, along with BH_99.
Cavallo et al. (2024)
Gold sample.