HSC 1082
0.28
UTI
0.46
CN
0.21
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad)
1.0 [N/pc2]
- CN 0.46 Poorly populated
- Cdens 0.21 Very loose
- CC3 0.75 High 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 1082 is a poorly populated, very loose object of high 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.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 44.226 | 71.019 | 1.133 | -0.889 | -2.063 | -29.373 |
| Liu et al. | 2025 | 44.38 | 70.98 | 1.12 | -0.97 | -2.07 | -19.79 |
| Cavallo et al. | 2024 | 43.752 | 71.056 | 1.126 | â | â | â |
| Hunt & Reffert | 2023 | 44.384 | 70.984 | 1.12 | -0.972 | -2.074 | -19.786 |
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 | 1.02 | 0.96 | 1.27 | 10 | 0.060 | â | â | â |
| Liu et al. | 2025 | 1.10 | 0.34 | â | 30 | â | â | â | â |
| Cavallo et al. | 2024 | 1.02 | 1.12 | â | 7 | 0.060 | â | â | â |
| Hunt & Reffert | 2023 | 0.85 | 0.96 | 1.27 | 10 | â | â | â | â |
Liu et al. (2025)
Classified as tidal capture (resonant trapping binary) 52 along with CWNU_77, and as primordial binary cluster 182 along with UBC_415, and of multiple system 22 along with CWNU_77, UBC_415 and FSR_0569.
Palma et al. (2025)
Part of multiple system G85, along with HSC_1052, CWNU_77, FSR_0569 and UBC_415.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.