OC 0292
0.26
UTI
0.32
CN
0.3
Cdens
0.25
CC3
0.31
Clit
0.88
Cdup
Radius (P>50% members)
9.3 [arcmin]
- CN 0.32 Poorly populated
- Cdens 0.3 Loose
- CC3 0.25 Low quality
- Clit 0.31 Poorly studied
- Cdup 0.88 Very likely unique
Overview
OC 0292 is a poorly populated, loose 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, young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is poorly studied in the literature.
Note: This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry. See table with shared members information.
Relatively close
Moderate extinction
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 85.543 | 36.125 | 0.582 | 0.642 | -3.023 | -19.699 |
| Zhang et al. | 2024 | 85.652 | 36.19 | â | â | â | â |
| Hunt & Reffert | 2024 | 85.652 | 36.19 | 0.575 | 0.651 | -2.946 | -4.695 |
| Cavallo et al. | 2024 | 85.55 | 36.097 | 0.578 | â | â | â |
| Hunt & Reffert | 2023 | 85.652 | 36.19 | 0.575 | 0.651 | -2.946 | -4.695 |
| Hao et al. | 2022 | 85.548 | 36.084 | 0.578 | 0.647 | -3.055 | -24.129 |
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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Zhang et al. | 2024 | â | â | â | â | -0.232* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 349* | â | â |
| Cavallo et al. | 2024 | 1.92 | 2.14 | â | 28 | 0.140 | â | â | â |
| Hunt & Reffert | 2023 | 1.59 | 1.76 | 2.73 | 50 | â | â | â | â |
| Hao et al. | 2022 | â | 1.73 | â | 1 | 0.611 | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Silver sample.