HSC 1293
0.04
UTI
0.0
CN
0.05
Cdens
0.25
CC3
0.25
Clit
0.24
Cdup
Stellar density (N50/rad)
0.2 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.05 Very loose
- CC3 0.25 Low quality
- Clit 0.25 Poorly studied
- Cdup 0.24 Likely duplicate
Overview
HSC 1293 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large distance, well below the mid-plane, affected by low extinction. It is catalogued as a metal-poor, old cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.
â ī¸ Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 63.79 | 32.273 | 0.188 | 0.264 | -0.662 | -12.101 |
| Hu & Soubiran | 2025 | 63.728 | 32.293 | â | â | â | â |
| Zhang et al. | 2024 | 63.804 | 32.296 | â | â | â | â |
| Cavallo et al. | 2024 | 63.728 | 32.293 | 0.18 | â | â | â |
| Hunt & Reffert | 2023 | 63.804 | 32.296 | 0.18 | 0.263 | -0.605 | -8.773 |
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 | 4.5 | 0.935 | 2.2 | 2210 | -0.527 | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.260(5) | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.527(1) | â | â | â |
| Cavallo et al. | 2024 | 4.53 | 1.07 | â | 2884 | -0.660 | â | â | â |
| Hunt & Reffert | 2023 | 4.47 | 0.80 | 2.20 | 1535 | 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.