HSC 2971
0.13
UTI
0.4
CN
0.14
Cdens
0.12
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
237.1 [arcmin]
- CN 0.4 Poorly populated
- Cdens 0.14 Very loose
- CC3 0.12 Very low quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
HSC 2971 is a poorly populated, very loose object of very low C3 quality. Its parallax locates it at a very 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.
Very close
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 | 255.755 | -25.665 | 9.052 | -4.222 | -6.135 | -23.605 |
| Cavallo et al. | 2024 | 255.841 | -23.436 | 9.297 | â | â | â |
| Hunt & Reffert | 2023 | 253.193 | -23.518 | 9.334 | -4.117 | -5.996 | -23.156 |
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 | 0.11 | 0.59 | â | 209 | -0.030 | â | â | â |
| Hunt & Reffert | 2023 | 0.10 | 0.10 | 0.42 | 238 | â | â | â | â |
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.