OC 0470
0.66
UTI
0.7
CN
1.0
Cdens
1.0
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members)
14.8 [arcmin]
- CN 0.7 Moderately populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.31 Poorly studied
- Cdup 1.0 Unique
Overview
OC 0470 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, very young 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 small percentage of members with at least one entry reported in the same catalogue. See table with shared members information.
Very close
Moderate extinction
Metal-rich
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 117.342 | -46.366 | 2.549 | -4.712 | 9.06 | 17.631 |
| Wei et al. | 2025 | 117.913 | -46.329 | 2.542 | -4.727 | 9.015 | â |
| Hunt & Reffert | 2024 | 117.375 | -46.368 | 2.54 | -4.684 | 8.975 | 15.103 |
| Cavallo et al. | 2024 | 117.462 | -46.684 | 2.539 | â | â | â |
| Hunt & Reffert | 2023 | 117.375 | -46.368 | 2.54 | -4.684 | 8.975 | 15.103 |
| Hao et al. | 2022 | 117.367 | -46.354 | 2.561 | -4.673 | 9.011 | 21.25 |
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 |
|---|---|---|---|---|---|---|---|---|---|
| Wei et al. | 2025 | 0.23 | 1.62 | â | 6 | 0.500 | 378 | 0.53 | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 198* | â | â |
| Cavallo et al. | 2024 | 0.40 | 0.77 | â | 4 | -0.250 | â | â | â |
| Hunt & Reffert | 2023 | 0.38 | 0.26 | 0.86 | 7 | â | â | â | â |
| Hao et al. | 2022 | â | 2.02 | â | 8 | 0.575 | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.