HSC 2418
0.09
UTI
0.0
CN
0.22
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
14.8 [arcmin]
- CN 0.0 Sparse
- Cdens 0.22 Very loose
- CC3 0.25 Low quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
HSC 2418 is a sparse, very loose object of low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low extinction. It is catalogued as an intermediate-age 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.
Relatively close
Low extinction
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 170.438 | -59.936 | 0.955 | -9.915 | 1.142 | -0.182 |
| Hunt & Reffert | 2023 | 170.181 | -60.041 | 0.961 | -9.895 | 1.112 | â |
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 | 2023 | 1.02 | 0.28 | 0.53 | 207 | â | â | â | â |
Hunt & Reffert (2024)
Classified as a moving group.