OC 0322
Summary
OC 0322 is a poorly populated, very dense object of very high C3 quality. It is located at a very close distance from the Sun, below 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 |
|---|---|---|---|---|---|---|
| Hao et al. (2022) | 79.413 | 7.153 | 2.552 | 2.356 | -3.735 | 14.728 |
| Hunt & Reffert (2023) | 79.418 | 7.164 | 2.55 | 2.291 | -3.666 | 6.219 |
| Cavallo et al. (2024) | 79.551 | 7.224 | 2.545 | – | – | – |
| UCC | 79.442 | 7.178 | 2.537 | 2.231 | -3.705 | 11.82 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hao et al. (2022) | AG=0.96, age=6.7, Z=0.025 |
| Hunt & Reffert (2023) | AV50=0.899, diffAV50=1.762, MOD50=7.873, logAge50=6.728 |
| Cavallo et al. (2024) | AV50=1.38, dMod50=8.18, logAge50=6.92, [Fe/H]50=0.17 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWNU 216 | 78.1 | 79.42 | 7.17 | 2.54 | 2.22 | -3.7 | 14.33 | 0.02 |
