CWNU 2450
Summary
CWNU 2450 is a sparse, loose object of low C3 quality. It is located at a moderate distance from the Sun, near 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) | 279.739 | -8.645 | 0.363 | -1.052 | -2.733 | 19.55 |
| UCC | 279.754 | -8.653 | 0.358 | -1.078 | -2.761 | 10.189 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=3.8, m-M=11.8, logAge=8.6 |
Search coordinates in Bayestar19