HSC 267
0.44
UTI
0.44
CN
1.0
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
7.0 [arcmin]
- CN 0.44 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
HSC 267 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 near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.
Relatively close
High 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 | 278.393 | -4.57 | 0.759 | 0.497 | -2.284 | -8.606 |
| Hunt & Reffert | 2024 | 278.417 | -4.552 | 0.727 | 0.511 | -2.267 | 1.178 |
| Cavallo et al. | 2024 | 278.392 | -4.577 | 0.738 | â | â | â |
| Hunt & Reffert | 2023 | 278.417 | -4.552 | 0.727 | 0.511 | -2.267 | 1.178 |
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 | 325* | â | â |
| Cavallo et al. | 2024 | 1.91 | 4.45 | â | 25 | 0.460 | â | â | â |
| Hunt & Reffert | 2023 | 1.28 | 3.93 | 2.71 | 48 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Bronze sample.