HSC 1490
0.05
UTI
0.0
CN
0.01
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
7.5 [arcmin]
- CN 0.0 Sparse
- Cdens 0.01 Very loose
- CC3 0.25 Low quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
HSC 1490 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large distance, well below the mid-plane, affected by moderate extinction. It is catalogued as an 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.
Very distant
Moderate extinction
Old
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 85.162 | 19.266 | 0.115 | 0.283 | -0.706 | -9.327 |
| Hunt & Reffert | 2023 | 85.197 | 19.239 | 0.102 | 0.277 | -0.694 | 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 | 9.03 | 1.46 | 1.27 | 1038 | â | â | â | â |
Hunt & Reffert (2024)
Classified as a moving group.