HSC 2047
0.00
UTI
0.26
CN
0.17
Cdens
0.12
CC3
0.0
Clit
0.04
Cdup
Radius (P>50% members)
56.8 [arcmin]
- CN 0.26 Poorly populated
- Cdens 0.17 Very loose
- CC3 0.12 Very low quality
- Clit 0.0 Rarely studied
- Cdup 0.04 Very likely duplicate
Overview
HSC 2047 is a poorly populated, very loose object of very low 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 (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
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 66.754 | -49.805 | 2.99 | 2.804 | 13.47 | 16.351 |
| Cavallo et al. | 2024 | 66.667 | -49.981 | 2.955 | â | â | â |
| Hunt & Reffert | 2023 | 64.457 | -48.445 | 2.944 | 2.972 | 13.311 | 13.241 |
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 | 0.34 | 0.24 | â | 32 | -0.040 | â | â | â |
| Hunt & Reffert | 2023 | 0.33 | 0.09 | 0.60 | 94 | â | â | â | â |
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.