HSC 2417
0.14
UTI
0.0
CN
0.1
Cdens
0.62
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
15.1 [arcmin]
- CN 0.0 Sparse
- Cdens 0.1 Very loose
- CC3 0.62 Intermediate quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
HSC 2417 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a 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.
Relatively close
Moderate extinction
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 166.662 | -64.195 | 0.694 | -6.535 | 4.981 | 7.971 |
| Cavallo et al. | 2024 | 166.671 | -64.21 | 0.686 | â | â | â |
| Hunt & Reffert | 2023 | 166.54 | -64.228 | 0.686 | -6.478 | 4.99 | 3.525 |
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 | 1.39 | 1.23 | â | 62 | -0.010 | â | â | â |
| Hunt & Reffert | 2023 | 1.40 | 1.09 | 1.25 | 38 | â | â | â | â |
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.