CWNU 3613
Summary
CWNU 3613 is a poorly populated, very loose object of high C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It was recently reported in the literature.
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) | 13.746 | 60.666 | 0.272 | -1.238 | -0.743 | – |
| UCC | 13.783 | 60.693 | 0.267 | -1.233 | -0.759 | -55.858 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.65, m-M=12.6, logA=7.6 |
Search coordinates in Bayestar19