HSC 572
0.17
UTI
0.25
CN
0.22
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad)
1.1 [N/pc2]
- CN 0.25 Poorly populated
- Cdens 0.22 Very loose
- CC3 0.38 Low quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
HSC 572 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a very close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the absorption parameter (see Parameters). It was recently reported in the literature.
Note: This object shares a moderate percentage of members with at least one entry reported in the same catalogue. See table with shared members information.
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.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 290.939 | 40.636 | 3.183 | -3.887 | 3.06 | -24.653 |
| Zhang et al. | 2024 | 290.682 | 40.622 | â | â | â | â |
| Cavallo et al. | 2024 | 290.459 | 39.919 | 3.121 | â | â | â |
| Hunt & Reffert | 2023 | 290.682 | 40.622 | 3.127 | -3.919 | 2.878 | -23.896 |
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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 0.32 | 0.24 | 0.35 | 76 | 0.038 | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | 0.036(1) | â | â | â |
| Cavallo et al. | 2024 | 0.33 | 0.46 | â | 47 | 0.040 | â | â | â |
| Hunt & Reffert | 2023 | 0.31 | 0.02 | 0.35 | 104 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.