HSC 592
0.07
UTI
0.0
CN
0.1
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
40.5 [arcmin]
- CN 0.0 Sparse
- Cdens 0.1 Very loose
- CC3 0.25 Low quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
HSC 592 is a sparse, very loose object of low C3 quality. Its parallax locates it at a close distance, above 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 | 298.794 | 40.442 | 1.794 | 5.039 | 5.666 | -16.242 |
| Zhang et al. | 2024 | 298.667 | 40.253 | â | â | â | â |
| Cavallo et al. | 2024 | 298.73 | 40.158 | 1.803 | â | â | â |
| Hunt & Reffert | 2023 | 298.667 | 40.253 | 1.809 | 5.055 | 5.703 | -15.527 |
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 | 0.077* | â | â | â |
| Cavallo et al. | 2024 | 0.58 | 0.54 | â | 155 | 0.320 | â | â | â |
| Hunt & Reffert | 2023 | 0.54 | 0.68 | 0.48 | 62 | 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.