HSC 1389
0.40
UTI
0.26
CN
1.0
Cdens
0.12
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members)
1.6 [arcmin]
- CN 0.26 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.12 Very low quality
- Clit 0.31 Poorly studied
- Cdup 1.0 Unique
Overview
HSC 1389 is a poorly populated, very dense object of very low C3 quality. Its parallax locates it at a moderate* distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, old cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.
(*): The parallax distance estimate (~4.56 kpc) differs significantly from the median photometric distance (~3.48 kpc).
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
Distant
Moderate extinction
Near-solar metallicity
Old
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 82.414 | 30.04 | 0.219 | 0.878 | 0.566 | -4.002 |
| Hu & Soubiran | 2025 | 82.418 | 30.054 | â | â | â | â |
| Zhang et al. | 2024 | 82.41 | 30.038 | â | â | â | â |
| Hunt & Reffert | 2024 | 82.41 | 30.038 | 0.233 | 0.896 | 0.609 | -3.996 |
| Cavallo et al. | 2024 | 82.418 | 30.054 | 0.234 | â | â | â |
| Hunt & Reffert | 2023 | 82.41 | 30.038 | 0.233 | 0.896 | 0.609 | -3.996 |
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 |
|---|---|---|---|---|---|---|---|---|---|
| Hu & Soubiran | 2025 | â | â | â | â | -0.160* | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.448* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 467* | â | â |
| Cavallo et al. | 2024 | 2.87 | 1.97 | â | 2089 | 0.220 | â | â | â |
| Hunt & Reffert | 2023 | 4.09 | 2.19 | 1.65 | 1312 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.