CWNU 1282
Summary
CWNU 1282 is a sparse, moderately dense 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) | 264.365 | -34.475 | 0.305 | -0.996 | -2.502 | – |
| UCC | 264.377 | -34.464 | 0.305 | -0.986 | -2.499 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=5.05, m-M=13.15, logAge=6.2 |
Search coordinates in Bayestar19