HSC 224
0.16
UTI
0.0
CN
0.16
Cdens
0.75
CC3
0.0
Clit
0.88
Cdup
Radius (P>50% members)
8.8 [arcmin]
- CN 0.0 Sparse
- Cdens 0.16 Very loose
- CC3 0.75 High quality
- Clit 0.0 Rarely studied
- Cdup 0.88 Very likely unique
Overview
HSC 224 is a sparse, very loose object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.
Note: This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry. See table with shared members information.
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=0.88) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Relatively close
Moderate extinction
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 280.244 | -11.76 | 0.558 | 0.67 | -0.71 | â |
| Hunt & Reffert | 2024 | 280.229 | -11.804 | 0.552 | 0.662 | -0.761 | -7.752 |
| Cavallo et al. | 2024 | 280.421 | -11.514 | 0.555 | â | â | â |
| Hunt & Reffert | 2023 | 280.229 | -11.804 | 0.552 | 0.662 | -0.761 | -7.752 |
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 | 2024 | â | â | â | â | â | 147* | â | â |
| Cavallo et al. | 2024 | 2.00 | 2.21 | â | 50 | 0.480 | â | â | â |
| Hunt & Reffert | 2023 | 1.68 | 1.97 | 2.46 | 64 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Gold sample.