HSC 296
0.15
UTI
0.0
CN
0.12
Cdens
0.62
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
19.5 [arcmin]
- CN 0.0 Sparse
- Cdens 0.12 Very loose
- CC3 0.62 Intermediate quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
HSC 296 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by moderate 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
Moderate 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 | 288.391 | -6.532 | 1.017 | -0.175 | -5.172 | 15.373 |
| Cavallo et al. | 2024 | 288.294 | -6.463 | 1.033 | â | â | â |
| Hunt & Reffert | 2023 | 288.445 | -6.344 | 1.026 | -0.2 | -5.142 | 9.438 |
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 | 1.02 | 1.68 | â | 178 | 0.300 | â | â | â |
| Hunt & Reffert | 2023 | 0.94 | 1.56 | 0.78 | 272 | â | â | â | â |
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.