HSC 1060
0.14
UTI
0.0
CN
0.04
Cdens
0.75
CC3
0.0
Clit
0.88
Cdup
Radius (P>50% members)
10.4 [arcmin]
- CN 0.0 Sparse
- Cdens 0.04 Very loose
- CC3 0.75 High quality
- Clit 0.0 Rarely studied
- Cdup 0.88 Very likely unique
Overview
HSC 1060 is a sparse, very loose object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a very metal-rich, young cluster (see Parameters). It was recently reported in the literature.
Note: This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry. See table with shared members information.
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=0.88) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Relatively close
Moderate extinction
Very metal-rich
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 29.519 | 61.913 | 0.341 | -1.027 | -0.391 | -15.47 |
| Hunt & Reffert | 2024 | 29.496 | 61.938 | 0.341 | -1.024 | -0.39 | -15.498 |
| Cavallo et al. | 2024 | 29.552 | 61.856 | 0.344 | â | â | â |
| Hunt & Reffert | 2023 | 29.496 | 61.938 | 0.341 | -1.024 | -0.39 | -15.498 |
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 |
|---|---|---|---|---|---|---|---|---|---|
| Hunt & Reffert | 2024 | â | â | â | â | â | 319* | â | â |
| Cavallo et al. | 2024 | 3.16 | 1.43 | â | 72 | 1.040 | â | â | â |
| Hunt & Reffert | 2023 | 2.65 | 1.86 | 1.79 | 24 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Gold sample.