HSC 1765
Summary
HSC 1765 is a poorly populated, very loose object of high C3 quality. It is located at a very close distance from the Sun, near the mid-plane. It was recently reported in the literature.This is a unique object, which shares a very small percentage of members with at least one previously reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Hunt & Reffert (2023) | 89.261 | -18.752 | 5.247 | -7.376 | 8.293 | 14.507 |
| Cavallo et al. (2024) | 87.578 | -18.931 | 5.244 | – | – | – |
| UCC | 87.561 | -18.777 | 5.237 | -7.435 | 8.088 | 16.686 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.08, diffAV50=0.39, MOD50=6.463, logAge50=7.589 |
| Cavallo et al. (2024) | AV50=0.59, dMod50=6.4, logAge50=7.63, [Fe/H]50=0.13 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWNU 1206 | 2.6 | 90.8 | -24.22 | 4.53 | -7.94 | 8.49 | 16.79 | 0.19 |
