CWNU 1099
(OCSN 119)
Summary
CWNU 1099 is a poorly populated, very dense 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 object shares a moderate percentage of members with a later reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| He et al. (2022) | 101.169 | -8.776 | 3.692 | -0.779 | -5.007 | – |
| Qin et al. (2023) | 101.48 | -9.51 | 3.48 | -0.68 | -4.46 | 28.26 |
| UCC | 101.144 | -8.724 | 3.65 | -0.774 | -4.995 | 27.856 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2022) | A0=0.25, logAge=7.45 |
| Qin et al. (2023) | E(B-V)=0.05, m-M=7.31, logt=7.45 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| Theia 72 | 30.3 | 101.7 | -9.78 | 3.46 | -0.95 | -4.33 | 25.83 | 0.23 |