OC 0413
0.00
UTI
0.28
CN
1.0
Cdens
0.75
CC3
0.31
Clit
0.0
Cdup
Radius (P>50% members)
1.9 [arcmin]
- CN 0.28 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.31 Poorly studied
- Cdup 0.0 Very likely duplicate
Overview
OC 0413 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, old cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is poorly studied in the literature.
â ī¸ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.
Distant
Moderate extinction
Near-solar metallicity
Old
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 108.706 | -26.245 | 0.271 | -2.071 | 2.762 | 79.813 |
| Hu & Soubiran | 2025 | 108.692 | -26.25 | â | â | â | â |
| Hunt & Reffert | 2024 | 108.695 | -26.247 | 0.27 | -2.08 | 2.77 | 80.108 |
| Cavallo et al. | 2024 | 108.692 | -26.25 | 0.27 | â | â | â |
| Hunt & Reffert | 2023 | 108.695 | -26.247 | 0.27 | -2.08 | 2.77 | 80.108 |
| Hao et al. | 2022 | 108.707 | -26.234 | 0.319 | -2.059 | 2.768 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Hu & Soubiran | 2025 | â | â | â | â | -0.200* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 550* | â | â |
| Cavallo et al. | 2024 | 3.13 | 0.96 | â | 1479 | 0.300 | â | â | â |
| Hunt & Reffert | 2023 | 3.47 | 1.08 | 1.74 | 1117 | â | â | â | â |
| Hao et al. | 2022 | â | 1.75 | â | 1000 | 0.370 | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.