HSC 1470
0.14
UTI
0.25
CN
0.33
Cdens
0.12
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
192.5 [arcmin]
- CN 0.25 Poorly populated
- Cdens 0.33 Loose
- CC3 0.12 Very low quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
HSC 1470 is a poorly populated, loose object of very low C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, old cluster (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
Moderate extinction
Near-solar metallicity
Old
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 81.107 | 20.697 | 14.294 | -9.917 | -30.817 | 15.735 |
| Cavallo et al. | 2024 | 81.267 | 19.872 | 15.272 | â | â | â |
| Hunt & Reffert | 2023 | 80.964 | 19.351 | 15.272 | -10.775 | -30.297 | 13.855 |
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 |
|---|---|---|---|---|---|---|---|---|---|
| Cavallo et al. | 2024 | 0.07 | 1.54 | â | 7244 | 0.320 | â | â | â |
| Hunt & Reffert | 2023 | 0.07 | 0.81 | 0.73 | 447 | â | â | â | â |
Cavallo et al. (2024)
Bronze sample.
Hunt & Reffert (2024)
Classified as a moving group.