CWNU 4139
Summary
CWNU 4139 is a sparse, very loose object of low 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) | 250.958 | -47.842 | 0.281 | -2.575 | -4.345 | -63.2 |
| UCC | 250.957 | -47.842 | 0.304 | -2.551 | -4.319 | -62.176 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=3.2, m-M=12.2, logA=8.7 |
Search coordinates in Bayestar19