HSC 2716
0.09
UTI
0.0
CN
0.21
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
24.6 [arcmin]
- CN 0.0 Sparse
- Cdens 0.21 Very loose
- CC3 0.25 Low quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
HSC 2716 is a sparse, very loose object of low C3 quality. Its parallax locates it at a close distance, below 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.
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 | 247.397 | -63.27 | 1.673 | 0.529 | -6.696 | -17.154 |
| Cavallo et al. | 2024 | 247.559 | -62.813 | 1.685 | â | â | â |
| Hunt & Reffert | 2023 | 246.803 | -63.461 | 1.687 | 0.635 | -6.551 | -9.127 |
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 | 0.61 | 0.53 | â | 120 | 0.050 | â | â | â |
| Hunt & Reffert | 2023 | 0.56 | 0.09 | 0.22 | 81 | â | â | â | â |
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.