CWNU 4419
Summary
CWNU 4419 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, below 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) | 276.587 | -22.534 | 0.194 | -1.301 | -6.798 | 116.48 |
| UCC | 276.582 | -22.534 | 0.167 | -1.355 | -6.838 | 116.481 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.85, m-M=12.8, logA=9.6 |
Search coordinates in Bayestar19