OC 0257
0.15
UTI
0.0
CN
0.15
Cdens
0.12
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad)
0.7 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.15 Very loose
- CC3 0.12 Very low quality
- Clit 0.25 Poorly studied
- Cdup 1.0 Unique
Overview
OC 0257 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is poorly studied in the literature.
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 46.058 | 59.297 | 1.192 | -0.182 | -1.433 | -14.009 |
| Hunt & Reffert | 2024 | 46.16 | 59.27 | 1.197 | -0.113 | -1.429 | -13.125 |
| Cavallo et al. | 2024 | 46.06 | 59.257 | 1.193 | â | â | â |
| Hunt & Reffert | 2023 | 46.16 | 59.27 | 1.197 | -0.113 | -1.429 | -13.125 |
| Hao et al. | 2022 | 46.179 | 59.255 | 1.186 | -0.267 | -1.278 | 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 | 0.82 | 1.61 | 0.79 | 316 | 0.420 | 79 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 79(1) | â | â |
| Cavallo et al. | 2024 | 0.82 | 1.34 | â | 355 | 0.230 | â | â | â |
| Hunt & Reffert | 2023 | 0.82 | 1.61 | 0.79 | 95 | â | â | â | â |
| Hao et al. | 2022 | â | 3.72 | â | 316 | 0.611 | 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.