HSC 2768
Summary
HSC 2768 is a poorly populated, very dense object of very high C3 quality. It is located at a moderate distance from the Sun, above the mid-plane. It was recently reported in the literature.
This object shares a large percentage of members with a later reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Hunt & Reffert (2023) | 243.916 | -48.645 | 0.219 | -2.851 | -3.24 | -69.257 |
| Hunt & Reffert (2024) | 243.916 | -48.645 | 0.219 | -2.851 | -3.24 | -69.257 |
| UCC | 243.921 | -48.64 | 0.228 | -2.875 | -3.238 | -69.26 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=5.501, diffAV50=1.881, MOD50=13.161, logAge50=8.213 |
| Hunt & Reffert (2024) | MassJ=1149.64, MassTot=1120.80 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWNU 3777 | 92.0 | 243.92 | -48.64 | 0.22 | -2.88 | -3.24 | -69.26 | 0.05 |
