CWNU 1892
Summary
CWNU 1892 is a sparse, very loose object of low C3 quality. It is located at a relatively close 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) | 125.408 | -43.712 | 0.618 | -4.588 | 4.136 | – |
| UCC | 125.398 | -43.661 | 0.618 | -4.584 | 4.136 | 18.975 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=2.1, m-M=11.15, logAge=7.95 |
Search coordinates in Bayestar19