HSC 295
0.11
UTI
0.31
CN
0.12
Cdens
0.12
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
62.8 [arcmin]
- CN 0.31 Poorly populated
- Cdens 0.12 Very loose
- CC3 0.12 Very low quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
HSC 295 is a poorly populated, very loose object of very low C3 quality. Its parallax locates it at a very close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Very close
Moderate extinction
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 273.88 | 0.977 | 2.569 | -1.261 | -13.683 | -15.472 |
| Zhang et al. | 2024 | 273.828 | 1.019 | â | â | â | â |
| Cavallo et al. | 2024 | 273.741 | 1.56 | 2.557 | â | â | â |
| Hunt & Reffert | 2023 | 273.828 | 1.019 | 2.542 | -1.357 | -13.352 | -15.187 |
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 | -0.018* | â | â | â |
| Cavallo et al. | 2024 | 0.40 | 1.19 | â | 263 | 0.480 | â | â | â |
| Hunt & Reffert | 2023 | 0.37 | 1.08 | 1.65 | 154 | 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.