HSC 2377
0.29
UTI
0.32
CN
0.37
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
4.6 [arcmin]
- CN 0.32 Poorly populated
- Cdens 0.37 Loose
- CC3 0.75 High quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
HSC 2377 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.
Relatively close
Moderate 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 | 163.085 | -58.737 | 0.32 | -6.013 | 2.702 | â |
| Hunt & Reffert | 2024 | 162.987 | -58.699 | 0.322 | -6.017 | 2.682 | â |
| Cavallo et al. | 2024 | 163.107 | -58.765 | 0.321 | â | â | â |
| Hunt & Reffert | 2023 | 162.987 | -58.699 | 0.322 | -6.017 | 2.682 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Hunt & Reffert | 2024 | â | â | â | â | â | 250* | â | â |
| Cavallo et al. | 2024 | 2.79 | 0.89 | â | 95 | 0.110 | â | â | â |
| Hunt & Reffert | 2023 | 2.74 | 1.22 | 2.32 | 94 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Silver sample.