HSC 1566
0.11
UTI
0.25
CN
0.17
Cdens
0.12
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
266.6 [arcmin]
- CN 0.25 Poorly populated
- Cdens 0.17 Very loose
- CC3 0.12 Very low quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
HSC 1566 is a poorly populated, very loose object of very low C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.
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.
Very close
Low 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 | 86.619 | -0.615 | 14.468 | 35.073 | -46.457 | 25.503 |
| Zhang et al. | 2024 | 80.653 | 5.338 | â | â | â | â |
| Cavallo et al. | 2024 | 86.277 | -0.385 | 15.199 | â | â | â |
| Hunt & Reffert | 2023 | 80.653 | 5.338 | 15.199 | 37.573 | -46.175 | 24.382 |
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 | 0.152* | â | â | â |
| Cavallo et al. | 2024 | 0.07 | 0.73 | â | 200 | -0.170 | â | â | â |
| Hunt & Reffert | 2023 | 0.07 | 0.11 | 0.68 | 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.
Hunt & Reffert (2024)
Classified as a moving group.