OC 0352
0.46
UTI
0.32
CN
1.0
Cdens
0.38
CC3
0.3
Clit
1.0
Cdup
Stellar density (N50/rad)
8.8 [N/pc2]
- CN 0.32 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.38 Low quality
- Clit 0.3 Poorly studied
- Cdup 1.0 Unique
Overview
OC 0352 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a relatively close distance, above 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 absorption 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.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 103.035 | 1.936 | 0.609 | -1.794 | 1.061 | â |
| Zhang et al. | 2024 | 103.023 | 1.916 | â | â | â | â |
| Hunt & Reffert | 2024 | 103.023 | 1.916 | 0.612 | -1.796 | 1.055 | â |
| Cavallo et al. | 2024 | 103.036 | 1.927 | 0.617 | â | â | â |
| Hunt & Reffert | 2023 | 103.023 | 1.916 | 0.612 | -1.796 | 1.055 | â |
| Hao et al. | 2022 | 103.027 | 1.921 | 0.62 | -1.783 | 1.026 | 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 | 1.535 | 1.03 | 1.01 | 501 | -0.090 | 203 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.376(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 203(1) | â | â |
| Cavallo et al. | 2024 | 1.56 | 1.03 | â | 339 | -0.090 | â | â | â |
| Hunt & Reffert | 2023 | 1.51 | 0.71 | 1.01 | 610 | â | â | â | â |
| Hao et al. | 2022 | â | 3.10 | â | 501 | 0.414 | 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.