HSC 570
0.09
UTI
0.0
CN
0.18
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad)
0.9 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.18 Very loose
- CC3 0.25 Low quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
đĨ Members
đ Colab
đŦ Bayestar19
MOCA
đ CDS
đ Simbad
đ CDS (Îą, δ)
đ Simbad (Îą, δ)
MOCA
đ CDS
đ Simbad
đ CDS (Îą, δ)
đ Simbad (Îą, δ)
Overview
HSC 570 is a sparse, 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, 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.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 285.447 | 42.095 | 4.078 | -0.55 | 2.269 | -19.428 |
| Zhang et al. | 2024 | 285.416 | 42.079 | â | â | â | â |
| Cavallo et al. | 2024 | 284.639 | 42.325 | 4.085 | â | â | â |
| Hunt & Reffert | 2023 | 285.416 | 42.079 | 4.078 | -0.678 | 2.285 | -17.716 |
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 | 0.25 | 0.265 | 0.2 | 144 | 0.168 | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | 0.125(1) | â | â | â |
| Cavallo et al. | 2024 | 0.26 | 0.49 | â | 58 | 0.210 | â | â | â |
| Hunt & Reffert | 2023 | 0.24 | 0.04 | 0.20 | 231 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
Palma et al. (2025)
Part of multiple system G182, along with HSC_558 and HSC_594.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.