HSC 598
0.06
UTI
0.26
CN
0.12
Cdens
0.38
CC3
0.0
Clit
0.38
Cdup
Radius (P>50% members)
122.3 [arcmin]
- CN 0.26 Poorly populated
- Cdens 0.12 Very loose
- CC3 0.38 Low quality
- Clit 0.0 Rarely studied
- Cdup 0.38 Possibly duplicate
Overview
HSC 598 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a very 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: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.
Very 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 | 335.012 | 13.286 | 5.308 | 15.507 | -11.201 | 5.541 |
| Zhang et al. | 2024 | 335.216 | 13.209 | â | â | â | â |
| Cavallo et al. | 2024 | 333.647 | 12.687 | 5.323 | â | â | â |
| Hunt & Reffert | 2023 | 335.216 | 13.209 | 5.353 | 15.604 | -11.264 | -1.368 |
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 | 0.031* | â | â | â |
| Cavallo et al. | 2024 | 0.19 | 0.43 | â | 89 | -0.030 | â | â | â |
| Hunt & Reffert | 2023 | 0.19 | 0.08 | 0.36 | 163 | 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.