HSC 1082
0.28
UTI
0.46
CN
0.21
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
25.9 [arcmin]
- CN 0.46 Poorly populated
- Cdens 0.21 Very loose
- CC3 0.75 High quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
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 moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.
Close
Moderate extinction
Near-solar metallicity
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 44.226 | 71.019 | 1.133 | -0.889 | -2.063 | -29.373 |
| 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| 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 |
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.