HSC 2147
0.11
UTI
0.0
CN
0.41
Cdens
0.12
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad)
2.1 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.41 Loose
- CC3 0.12 Very low quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
HSC 2147 is a sparse, loose object of very low C3 quality. Its parallax locates it at a close 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.
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 | 130.862 | -47.316 | 1.386 | -8.284 | 4.2 | 30.829 |
| Cavallo et al. | 2024 | 130.742 | -47.366 | 1.392 | â | â | â |
| Hunt & Reffert | 2023 | 131.177 | -47.336 | 1.391 | -8.233 | 4.232 | 33.584 |
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 | 0.635 | 0.54 | 0.43 | 152 | -0.470 | â | â | â |
| Cavallo et al. | 2024 | 0.59 | 0.85 | â | 229 | -0.470 | â | â | â |
| Hunt & Reffert | 2023 | 0.68 | 0.23 | 0.43 | 74 | â | â | â | â |
MOCA


Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.