CWNU 1090
(OCSN 174)
Summary
CWNU 1090 is a rich, dense object of high C3 quality. It is located at a very close distance from the Sun, above the mid-plane. It was recently reported in the literature.
This object shares a small percentage of members with a later reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| He et al. (2022) | 0.948 | 79.696 | 6.491 | 22.848 | 0.259 | – |
| Qin et al. (2023) | 8.28 | 79.61 | 6.34 | 23.02 | -2.33 | -8.41 |
| UCC | 343.28 | 79.472 | 6.399 | 22.619 | 0.28 | -8.774 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2022) | A0=0.05, logAge=7.25 |
| Qin et al. (2023) | E(B-V)=0.05, m-M=6.13, logt=7.2 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| HSC 976 | 11.2 | 343.74 | 78.44 | 6.0 | 18.56 | 5.91 | -8.58 | 0.32 |