OC 0290
0.12
UTI
0.0
CN
0.2
Cdens
0.25
CC3
0.06
Clit
1.0
Cdup
Nm (P>50%)
23
Core radius and density
2.0 [pc], 1.0 [pc-2]
- CN 0.0 Sparse
- Cdens 0.2 Very loose
- CC3 0.25 Low quality
- Clit 0.06 Rarely studied
- Cdup 1.0 Unique
Overview
OC 0290 is a sparse, very loose object of low C3 quality. Its parallax locates it at a relatively close distance, below 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 metallicity parameter (see Parameters). It is rarely 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 | 75.404 | 30.741 | 0.579 | 0.766 | -2.972 | 30.664 |
| Hunt & Reffert | 2024 | 75.435 | 30.759 | 0.574 | 0.791 | -2.995 | 30.602 |
| Cavallo et al. | 2024 | 75.405 | 30.743 | 0.573 | â | â | â |
| Hunt & Reffert | 2023 | 75.435 | 30.759 | 0.574 | 0.791 | -2.995 | 30.602 |
| Hao et al. | 2022 | 75.376 | 30.739 | 0.587 | 0.764 | -3.018 | 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 | 1.62 | 1.63 | 1.36 | 454 | 0.281 | 133 | â | â |
| Hunt & Reffert | 2024 | 1.62 | 1.63 | 1.36 | 511 | â | 133(1) | â | â |
| Cavallo et al. | 2024 | 2.06 | 1.95 | â | 282 | 0.490 | â | â | â |
| Hunt & Reffert | 2023 | 1.62 | 1.63 | 1.36 | 511 | â | â | â | â |
| Hao et al. | 2022 | â | 1.04 | â | 398 | 0.073 | 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.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.19 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.19 (50th percentile).