OC 0124
0.07
UTI
0.58
CN
1.0
Cdens
0.75
CC3
0.25
Clit
0.12
Cdup
Stellar density (N50/rad)
12.7 [N/pc2]
- CN 0.58 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.25 Poorly studied
- Cdup 0.12 Likely duplicate
Overview
OC 0124 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is poorly studied in the literature.
â ī¸ Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry, and a small percentage with at least one entry reported in the same catalogue. 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 | 306.406 | 40.908 | 0.511 | -3.095 | -4.179 | 45.724 |
| Hunt & Reffert | 2024 | 306.438 | 40.924 | 0.491 | -3.115 | -4.137 | 45.631 |
| Cavallo et al. | 2024 | 306.409 | 40.914 | 0.492 | â | â | â |
| Hunt & Reffert | 2023 | 306.438 | 40.924 | 0.491 | -3.115 | -4.137 | 45.631 |
| Hao et al. | 2022 | 306.448 | 40.911 | 0.546 | -3.017 | -4.558 | 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 | 1.63 | 3.04 | 2.18 | 64 | 0.066 | 380 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 380(1) | â | â |
| Cavallo et al. | 2024 | 1.36 | 3.06 | â | 123 | -0.480 | â | â | â |
| Hunt & Reffert | 2023 | 1.90 | 3.04 | 2.18 | 64 | â | â | â | â |
| Hao et al. | 2022 | â | 1.85 | â | 16 | 0.611 | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Palma et al. (2025)
Part of multiple system G71, along with Dolidze_11 and FSR_0227.
Cavallo et al. (2024)
Gold sample.