HSC 2018
0.24
UTI
0.31
CN
0.24
Cdens
0.62
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
17.8 [arcmin]
- CN 0.31 Poorly populated
- Cdens 0.24 Very loose
- CC3 0.62 Intermediate quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
HSC 2018 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low extinction. It is catalogued as a low-mass, near-solar metallicity, young 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.
Close
Low extinction
Low mass
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 122.624 | -33.016 | 1.025 | -5.752 | 6.901 | 35.37 |
| Hunt & Reffert | 2024 | 122.687 | -33.062 | 1.023 | -5.732 | 6.886 | 36.054 |
| Cavallo et al. | 2024 | 122.514 | -32.844 | 1.025 | â | â | â |
| Hunt & Reffert | 2023 | 122.687 | -33.062 | 1.023 | -5.732 | 6.886 | 36.054 |
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 | 48* | â | â |
| Cavallo et al. | 2024 | 0.99 | 0.52 | â | 68 | -0.050 | â | â | â |
| Hunt & Reffert | 2023 | 0.93 | 0.34 | 0.78 | 100 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Gold sample.