HSC 1426
0.11
UTI
0.25
CN
1.0
Cdens
1.0
CC3
0.25
Clit
0.2
Cdup
Stellar density (N50/rad)
8.3 [N/pc2]
- CN 0.25 Poorly populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.25 Poorly studied
- Cdup 0.2 Likely duplicate
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 1426 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a very close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the absorption 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 | 56.523 | 6.051 | 5.463 | 21.204 | -13.456 | 16.793 |
| Liu et al. | 2025 | 56.48 | 5.94 | 5.35 | 20.25 | -12.98 | 16.46 |
| Zhang et al. | 2024 | 56.478 | 5.943 | â | â | â | â |
| Cavallo et al. | 2024 | 58.235 | 5.2 | 5.397 | â | â | â |
| Hunt & Reffert | 2023 | 56.478 | 5.943 | 5.345 | 20.251 | -12.985 | 16.457 |
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 | 0.19 | 0.13 | 0.34 | 49 | 0.012 | â | â | â |
| Liu et al. | 2025 | 0.22 | 0.13 | â | 45 | â | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.036(1) | â | â | â |
| Cavallo et al. | 2024 | 0.19 | 0.93 | â | 49 | 0.060 | â | â | â |
| Hunt & Reffert | 2023 | 0.18 | 0.12 | 0.34 | 80 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
Liu et al. (2025)
Classified as primordial binary cluster 193 along with HSC_1438, and of multiple system 35 along with Theia_71, HSC_1438, CWNU_1129, Theia_54 and Theia_66.
Palma et al. (2025)
Part of multiple system G115, along with HSC_1373 and HSC_1438.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.