HSC 1097
0.12
UTI
0.0
CN
0.09
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad)
0.5 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.09 Very loose
- CC3 0.5 Intermediate 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 1097 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane. It is catalogued as a low-mass, near-solar metallicity 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 | 30.222 | 47.976 | 0.512 | 3.402 | -1.453 | 29.987 |
| Zhang et al. | 2024 | 30.169 | 48.026 | â | â | â | â |
| Hunt & Reffert | 2024 | 30.169 | 48.026 | 0.51 | 3.37 | -1.43 | 25.39 |
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 | â | â | â | â | -0.197 | 46 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.197(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 46(1) | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
