CWNU 1949
Summary
CWNU 1949 is a sparse, very loose object of very low C3 quality. It is located at a moderate distance from the Sun, well 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) | 153.6 | -47.487 | 0.271 | -5.425 | 3.563 | 60.95 |
| UCC | 153.671 | -47.564 | 0.247 | -5.415 | 3.563 | 50.579 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=0.5, m-M=12.95, logAge=9.5 |
Search coordinates in Bayestar19