UBC 372
0.10
UTI
0.68
CN
1.0
Cdens
1.0
CC3
0.38
Clit
0.14
Cdup
Radius (P>50% members)
2.1 [arcmin]
- CN 0.68 Moderately populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.38 Poorly studied
- Cdup 0.14 Likely duplicate
Overview
UBC 372 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (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. See table with shared members information.
Distant
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 | 302.38 | 38.291 | 0.271 | -2.584 | -4.875 | â |
| Zhang et al. | 2024 | 302.37 | 38.289 | â | â | â | â |
| Hunt & Reffert | 2024 | 302.37 | 38.289 | 0.261 | -2.595 | -4.867 | â |
| Cavallo et al. | 2024 | 302.384 | 38.284 | 0.266 | â | â | â |
| Hunt & Reffert | 2023 | 302.37 | 38.289 | 0.261 | -2.595 | -4.867 | â |
| Cantat-Gaudin et al. | 2020 | 302.375 | 38.291 | 0.255 | -2.601 | -4.885 | â |
| Castro-Ginard et al. | 2020 | 302.368 | 38.283 | 0.261 | -2.609 | -4.891 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Zhang et al. | 2024 | â | â | â | â | 0.134* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 566* | â | â |
| Cavallo et al. | 2024 | 3.02 | 2.43 | â | 91 | -0.100 | â | â | â |
| Hunt & Reffert | 2023 | 3.31 | 2.15 | 0.62 | 71 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 3.24 | 1.90 | â | 115 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.