CWNU 4607
Summary
CWNU 4607 is a sparse, very loose object of intermediate C3 quality. It is located at a large distance from the Sun, well 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) | 274.709 | -30.133 | 0.152 | -1.194 | -3.812 | -37.84 |
| UCC | 274.704 | -30.127 | 0.143 | -1.18 | -3.812 | -37.839 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.2, m-M=13.7, logA=9.2 |
Search coordinates in Bayestar19