HSC 1943
0.13
UTI
0.0
CN
0.27
Cdens
0.5
CC3
0.0
Clit
0.88
Cdup
Radius (P>50% members)
3.0 [arcmin]
- CN 0.0 Sparse
- Cdens 0.27 Loose
- CC3 0.5 Intermediate quality
- Clit 0.0 Rarely studied
- Cdup 0.88 Very likely unique
Overview
HSC 1943 is a sparse, loose object of intermediate 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, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Note: This is very likely a unique object, which shares a small 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=0.88) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Distant
Low extinction
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 116.968 | -25.88 | 0.231 | -1.908 | 2.354 | â |
| Hunt & Reffert | 2024 | 116.958 | -25.883 | 0.23 | -1.926 | 2.365 | â |
| Cavallo et al. | 2024 | 116.948 | -25.868 | 0.229 | â | â | â |
| Hunt & Reffert | 2023 | 116.958 | -25.883 | 0.23 | -1.926 | 2.365 | 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 | 2024 | â | â | â | â | â | 136* | â | â |
| Cavallo et al. | 2024 | 3.08 | 1.29 | â | 129 | -0.310 | â | â | â |
| Hunt & Reffert | 2023 | 3.96 | 0.65 | 0.70 | 175 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Gold sample.