CWNU 1450
Summary
CWNU 1450 is a poorly populated, very loose object of low C3 quality. It is located at a relatively close distance from the Sun, below the mid-plane. It was recently reported in the literature.
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) | 4.654 | 56.272 | 0.532 | -2.748 | -2.365 | – |
| UCC | 4.591 | 56.272 | 0.512 | -2.746 | -2.356 | -30.569 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.4, m-M=11.5, logAge=7.6 |
Search coordinates in Bayestar19