CWNU 3601
Summary
CWNU 3601 is a sparse, very loose object of high C3 quality. It is located at a large 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) | 107.628 | -16.7 | 0.13 | -0.624 | 1.223 | – |
| UCC | 107.594 | -16.719 | 0.13 | -0.635 | 1.234 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=2.15, m-M=15.65, logA=6.7 |
Search coordinates in Bayestar19