HSC 263
0.13
UTI
0.0
CN
0.17
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad)
0.8 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.17 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 263 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very young 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 | 264.748 | 2.468 | 1.91 | 0.062 | -9.264 | -11.222 |
| Zhang et al. | 2024 | 264.822 | 2.426 | â | â | â | â |
| Cavallo et al. | 2024 | 264.086 | 2.638 | 1.92 | â | â | â |
| Hunt & Reffert | 2023 | 264.822 | 2.426 | 1.909 | 0.04 | -9.345 | -12.792 |
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 | 0.53 | 0.675 | 0.54 | 17 | 0.097 | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | 0.174(1) | â | â | â |
| Cavallo et al. | 2024 | 0.57 | 0.98 | â | 8 | 0.020 | â | â | â |
| Hunt & Reffert | 2023 | 0.49 | 0.37 | 0.54 | 26 | 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.