HSC 2356
0.00
UTI
0.0
CN
1.0
Cdens
0.75
CC3
0.0
Clit
0.0
Cdup
Radius (P>50% members)
9.8 [arcmin]
- CN 0.0 Sparse
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.0 Rarely studied
- Cdup 0.0 Very likely duplicate
Overview
HSC 2356 is a sparse, very dense object of high C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.
â ī¸ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.
Very close
Low extinction
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 159.484 | -59.034 | 2.047 | -14.64 | 0.997 | -11.524 |
| Wei et al. | 2025 | 159.468 | -59.082 | 2.234 | -14.478 | 1.049 | â |
| Hunt & Reffert | 2023 | 159.587 | -58.978 | 1.9 | -14.658 | 0.942 | â |
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 |
|---|---|---|---|---|---|---|---|---|---|
| Wei et al. | 2025 | 0.42 | 0.11 | â | 65 | 0.250 | 812 | 0.36 | â |
| Hunt & Reffert | 2023 | 0.53 | 1.89 | 0.64 | 417 | â | â | â | â |
Hunt & Reffert (2024)
Classified as a moving group.