HSC 912
0.24
UTI
0.25
CN
0.2
Cdens
0.25
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members)
14.1 [arcmin]
- CN 0.25 Poorly populated
- Cdens 0.2 Very loose
- CC3 0.25 Low quality
- Clit 0.25 Poorly studied
- Cdup 1.0 Unique
Overview
HSC 912 is a poorly populated, very loose object of low 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, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Relatively close
High 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 | 349.63 | 66.606 | 0.822 | 0.196 | -2.051 | -14.519 |
| Hu & Soubiran | 2025 | 349.612 | 66.57 | â | â | â | â |
| Hunt & Reffert | 2024 | 349.715 | 66.646 | 0.817 | 0.232 | -2.044 | -12.438 |
| Cavallo et al. | 2024 | 349.612 | 66.57 | 0.824 | â | â | â |
| Hunt & Reffert | 2023 | 349.715 | 66.646 | 0.817 | 0.232 | -2.044 | -12.438 |
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 | -0.110* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 103* | â | â |
| Cavallo et al. | 2024 | 1.25 | 3.13 | â | 708 | -0.170 | â | â | â |
| Hunt & Reffert | 2023 | 1.20 | 3.24 | 2.01 | 79 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Gold sample.