HSC 1176
0.18
UTI
0.25
CN
0.17
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
28.0 [arcmin]
- CN 0.25 Poorly populated
- Cdens 0.17 Very loose
- CC3 0.5 Intermediate quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
HSC 1176 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (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.
Close
Low 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 | 41.508 | 37.767 | 1.506 | -2.89 | -1.861 | -21.099 |
| Zhang et al. | 2024 | 41.526 | 37.788 | â | â | â | â |
| Cavallo et al. | 2024 | 41.191 | 37.87 | 1.482 | â | â | â |
| Hunt & Reffert | 2023 | 41.526 | 37.788 | 1.473 | -2.902 | -1.875 | -17.844 |
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 | -0.028* | â | â | â |
| Cavallo et al. | 2024 | 0.66 | 0.09 | â | 251 | 0.270 | â | â | â |
| Hunt & Reffert | 2023 | 0.63 | 0.12 | 0.48 | 124 | 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.