CWWDL 5475
Summary
CWWDL 5475 is a poorly populated, very dense object of high C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It was recently reported 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 |
|---|---|---|---|---|---|---|
| Chi et al. (2023) | 198.196 | -64.259 | 0.447 | -4.399 | -0.497 | -25.611 |
| UCC | 198.218 | -64.265 | 0.459 | -4.354 | -0.522 | -18.401 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Chi et al. (2023) | logAge=7.88, Z=-0.28 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| LISC 3164 | 100.0 | 198.23 | -64.26 | 0.46 | -4.34 | -0.54 | -18.4 | 0.49 |
| UBC 1522 | 100.0 | 198.22 | -64.26 | 0.46 | -4.35 | -0.53 | -18.4 | 0.02 |
| CWNU 278 | 51.1 | 198.22 | -64.26 | 0.45 | -4.35 | -0.53 | -15.14 | 0.0 |