CWNU 1419
Summary
CWNU 1419 is a sparse, very loose object of very 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: 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) | 123.291 | -39.846 | 0.508 | -2.872 | 3.384 | – |
| UCC | 123.288 | -39.844 | 0.502 | -2.88 | 3.383 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=2.15, m-M=11.55, logAge=7.0 |
Search coordinates in Bayestar19