CWNU 4449
Summary
CWNU 4449 is a sparse, very loose object of intermediate C3 quality. It is located at a moderate 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) | 254.016 | -40.967 | 0.22 | -1.392 | -2.83 | -30.88 |
| UCC | 254.015 | -40.97 | 0.218 | -1.451 | -2.814 | -73.824 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=5.8, m-M=12.55, logA=8.7 |
Search coordinates in Bayestar19