HSC 1788
0.07
UTI
0.0
CN
0.03
Cdens
0.25
CC3
0.03
Clit
1.0
Cdup
Nm (P>50%)
19
Core radius and density
4.1 [pc], 0.1 [pc-2]
- CN 0.0 Sparse
- Cdens 0.03 Very loose
- CC3 0.25 Low quality
- Clit 0.03 Rarely studied
- Cdup 1.0 Unique
Overview
HSC 1788 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, near 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.
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
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.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 109.133 | -12.507 | 0.29 | -2.069 | 2.152 | â |
| Hunt & Reffert | 2024 | 109.14 | -12.559 | 0.283 | -2.063 | 2.164 | â |
| Cavallo et al. | 2024 | 109.16 | -12.507 | 0.286 | â | â | â |
| Hunt & Reffert | 2023 | 109.14 | -12.559 | 0.283 | -2.063 | 2.164 | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 3.02 | 1.41 | 0.47 | 93 | 0.130 | 149 | â | â |
| Hunt & Reffert | 2024 | 3.02 | 1.41 | 0.47 | 93 | â | 149(1) | â | â |
| Cavallo et al. | 2024 | 2.82 | 1.31 | â | 148 | 0.130 | â | â | â |
| Hunt & Reffert | 2023 | 3.02 | 1.41 | 0.47 | 93 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 1.00 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (50th percentile).