HSC 2005
0.02
UTI
0.0
CN
0.08
Cdens
0.0
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
12.0 [arcmin]
- CN 0.0 Sparse
- Cdens 0.08 Very loose
- CC3 0.0 Very low quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
HSC 2005 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by low extinction. It is catalogued as a very old 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.
Relatively close
Low extinction
Very old
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 126.147 | -28.755 | 0.459 | -3.16 | -2.836 | â |
| Hunt & Reffert | 2023 | 126.132 | -28.778 | 0.477 | -3.304 | -2.753 | 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 | 2023 | 1.95 | 0.14 | 0.66 | 8650 | â | â | â | â |
Hunt & Reffert (2024)
Classified as a moving group.