CWNU 4822
Summary
CWNU 4822 is a sparse, very loose object of low 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) | 299.746 | 21.614 | 0.148 | -2.501 | -4.803 | – |
| UCC | 299.746 | 21.614 | 0.129 | -2.497 | -4.803 | -6.675 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=0.55, m-M=16.1, logA=10.1 |
Search coordinates in Bayestar19