CWNU 1912
Summary
CWNU 1912 is a sparse, very loose object of intermediate C3 quality. It is located at a moderate 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) | 145.156 | -56.948 | 0.386 | -5.398 | 4.097 | -0.82 |
| UCC | 145.255 | -56.972 | 0.383 | -5.396 | 4.071 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.55, m-M=11.9, logAge=8.1 |
Search coordinates in Bayestar19