HSC 2635
0.44
UTI
0.47
CN
1.0
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
2.5 [arcmin]
- CN 0.47 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
HSC 2635 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a metal-rich, young cluster (see Parameters). It was recently reported in the literature.
Distant
High extinction
Metal-rich
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 210.83 | -59.67 | 0.33 | -4.681 | -1.778 | -32.904 |
| Hunt & Reffert | 2024 | 210.827 | -59.669 | 0.328 | -4.69 | -1.8 | â |
| Cavallo et al. | 2024 | 210.817 | -59.667 | 0.329 | â | â | â |
| Hunt & Reffert | 2023 | 210.827 | -59.669 | 0.328 | -4.69 | -1.8 | 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 | 396* | â | â |
| Cavallo et al. | 2024 | 3.80 | 3.33 | â | 148 | 0.610 | â | â | â |
| Hunt & Reffert | 2023 | 2.60 | 3.08 | 2.96 | 40 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Silver sample.