OC 0290
Summary
OC 0290 is a sparse, very dense object of low C3 quality. It is located at a relatively 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.
Warning: contains less than 25 stars with P>0.5 estimated.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Hao et al. (2022) | 75.376 | 30.739 | 0.587 | 0.764 | -3.018 | – |
| Hunt & Reffert (2023) | 75.435 | 30.759 | 0.574 | 0.791 | -2.995 | 30.602 |
| Cavallo et al. (2024) | 75.405 | 30.743 | 0.573 | – | – | – |
| Hunt & Reffert (2024) | 75.435 | 30.759 | 0.574 | 0.791 | -2.995 | 30.602 |
| UCC | 75.404 | 30.741 | 0.579 | 0.766 | -2.972 | 30.664 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hao et al. (2022) | AG=0.82, age=8.6, Z=0.018 |
| Hunt & Reffert (2023) | AV50=1.632, diffAV50=1.361, MOD50=11.051, logAge50=8.708 |
| Cavallo et al. (2024) | AV50=1.95, dMod50=11.57, logAge50=8.45, [Fe/H]50=0.49 |
| Hunt & Reffert (2024) | MassJ=133.327, MassTot=134.654 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWNU 344 | 92.0 | 75.41 | 30.75 | 0.58 | 0.76 | -2.97 | 24.22 | 0.04 |
