CWNU 4404
Summary
CWNU 4404 is a sparse, very loose object of high C3 quality. It is located at a very large distance from the Sun, above the mid-plane. It was recently reported in the literature.
Warning: contains less than 25 stars with P>0.5 estimated.
Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicates that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| He et al. (2023) | 219.713 | -58.612 | 0.111 | -5.276 | -2.559 | 39.47 |
| UCC | 219.706 | -58.618 | 0.093 | -5.27 | -2.598 | 21.334 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=5.0, m-M=16.3, logA=8.5 |
Search coordinates in Bayestar19