HSC 1752
0.03
UTI
0.0
CN
0.05
Cdens
0.38
CC3
0.0
Clit
0.4
Cdup
Radius (P>50% members)
10.1 [arcmin]
- CN 0.0 Sparse
- Cdens 0.05 Very loose
- CC3 0.38 Low quality
- Clit 0.0 Rarely studied
- Cdup 0.4 Possibly duplicate
Overview
HSC 1752 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.
â ī¸ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=0.4) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Relatively close
Low 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 | 107.815 | -8.394 | 0.371 | -1.215 | 1.0 | 97.513 |
| Cavallo et al. | 2024 | 107.829 | -8.371 | 0.35 | â | â | â |
| Hunt & Reffert | 2023 | 107.835 | -8.409 | 0.349 | -1.195 | 1.008 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Cavallo et al. | 2024 | 2.48 | 0.90 | â | 12 | -0.350 | â | â | â |
| Hunt & Reffert | 2023 | 2.50 | 0.69 | 1.11 | 47 | â | â | â | â |
Cavallo et al. (2024)
Gold sample.