UBC 385
Summary
UBC 385 is a poorly populated, very dense object of very high C3 quality. It is located at a close distance from the Sun, above the mid-plane. It is poorly studied in the literature.
Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Castro-Ginard et al. (2020) | 317.945 | 60.077 | 1.18 | -2.538 | -3.466 | – |
| Cantat-Gaudin et al. (2020) | 317.94 | 60.092 | 1.178 | -2.53 | -3.468 | – |
| He et al. (2022) | 317.952 | 60.014 | 1.187 | -2.521 | -3.517 | – |
| Celli et al. (2024) | 317.94 | 60.092 | – | – | – | – |
| Alfonso et al. (2024) | 318.434 | 59.506 | 1.116 | -2.553 | -3.558 | – |
| UCC | 317.944 | 60.023 | 1.176 | -2.531 | -3.506 | -17.856 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Cantat-Gaudin et al. (2020) | AVNN=1.2, DistPc=876.0, AgeNN=7.29 |
| He et al. (2022) | A0=1.55, logAge=6.9 |
| Celli et al. (2024) | Age=19.5, Mc=141.6 |
| Alfonso et al. (2024) | AV=1.19907, MOD=9.70984, logAge=7.61589, Z=0.01004 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| Riddle 6 | 100.0 | 318.03 | 59.9 | 1.17 | -2.53 | -3.51 | -23.22 | 0.71 |
| OC 0158 | 14.3 | 318.24 | 59.51 | 1.16 | -2.54 | -3.51 | -24.65 | 0.03 |
| CWNU 1192 | 5.7 | 318.54 | 59.41 | 1.16 | -2.51 | -3.5 | -25.37 | 0.02 |
