HSC 474
0.09
UTI
0.32
CN
0.29
Cdens
0.62
CC3
0.0
Clit
0.38
Cdup
Radius (P>50% members)
48.0 [arcmin]
- CN 0.32 Poorly populated
- Cdens 0.29 Loose
- CC3 0.62 Intermediate quality
- Clit 0.0 Rarely studied
- Cdup 0.38 Possibly duplicate
Overview
HSC 474 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a very close distance, above 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 possibly a duplicate object, which shares a significant 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 | 264.434 | 35.899 | 2.993 | -2.715 | -3.342 | -23.91 |
| Zhang et al. | 2024 | 260.805 | 34.708 | â | â | â | â |
| Cavallo et al. | 2024 | 263.256 | 35.153 | 3.106 | â | â | â |
| Hunt & Reffert | 2023 | 260.805 | 34.708 | 3.076 | -2.848 | -3.864 | -22.208 |
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 |
|---|---|---|---|---|---|---|---|---|---|
| Zhang et al. | 2024 | â | â | â | â | 0.103* | â | â | â |
| Cavallo et al. | 2024 | 0.34 | 0.45 | â | 17 | -0.090 | â | â | â |
| Hunt & Reffert | 2023 | 0.31 | 0.09 | 0.63 | 31 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.