HSC 2760
0.43
UTI
0.38
CN
1.0
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
1.7 [arcmin]
- CN 0.38 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
HSC 2760 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a relatively close 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.
Relatively close
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 | 242.306 | -48.924 | 0.528 | 0.533 | -0.972 | 108.959 |
| Hunt & Reffert | 2024 | 242.309 | -48.929 | 0.551 | 0.529 | -0.985 | 108.96 |
| Cavallo et al. | 2024 | 242.359 | -48.919 | 0.524 | â | â | â |
| Hunt & Reffert | 2023 | 242.309 | -48.929 | 0.551 | 0.529 | -0.985 | 108.96 |
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 | 227* | â | â |
| Cavallo et al. | 2024 | 2.05 | 3.65 | â | 24 | 0.510 | â | â | â |
| Hunt & Reffert | 2023 | 1.74 | 3.54 | 2.61 | 51 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Silver sample.