OC 0175
0.00
UTI
0.45
CN
1.0
Cdens
0.25
CC3
0.31
Clit
0.0
Cdup
Radius (P>50% members)
2.1 [arcmin]
- CN 0.45 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.25 Low quality
- Clit 0.31 Poorly studied
- Cdup 0.0 Very likely duplicate
Overview
OC 0175 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (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.
Relatively close
Moderate extinction
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 334.716 | 57.436 | 0.321 | -4.391 | -3.587 | -72.644 |
| Hu & Soubiran | 2025 | 334.736 | 57.435 | â | â | â | â |
| Hunt & Reffert | 2024 | 334.722 | 57.435 | 0.313 | -4.383 | -3.565 | -72.641 |
| Cavallo et al. | 2024 | 334.736 | 57.435 | 0.314 | â | â | â |
| Hunt & Reffert | 2023 | 334.722 | 57.435 | 0.313 | -4.383 | -3.565 | -72.641 |
| Hao et al. | 2022 | 334.752 | 57.43 | 0.325 | -4.409 | -3.561 | -75.146 |
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 | -0.150* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 780* | â | â |
| Cavallo et al. | 2024 | 2.43 | 2.76 | â | 676 | 0.060 | â | â | â |
| Hunt & Reffert | 2023 | 2.88 | 2.84 | 1.95 | 288 | â | â | â | â |
| Hao et al. | 2022 | â | 3.62 | â | 631 | 0.274 | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.