HSC 113
0.10
UTI
0.0
CN
0.01
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad)
0.1 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.01 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 113 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a large distance, well below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, old cluster, but with a large variance across recent sources for the age parameter (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 | 279.765 | -26.545 | 0.117 | -3.97 | -4.644 | -44.246 |
| Hu & Soubiran | 2025 | 279.75 | -26.543 | â | â | â | â |
| Cavallo et al. | 2024 | 279.75 | -26.543 | 0.122 | â | â | â |
| Hunt & Reffert | 2023 | 279.771 | -26.557 | 0.122 | -3.924 | -4.684 | -6.954 |
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 | 7.125 | 1.435 | 1.35 | 4326 | -0.345 | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.300(5) | â | â | â |
| Cavallo et al. | 2024 | 7.28 | 1.18 | â | 7079 | -0.390 | â | â | â |
| Hunt & Reffert | 2023 | 6.97 | 1.69 | 1.35 | 1574 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.