CWNU 4174
Summary
CWNU 4174 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, above 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) | 332.328 | 60.35 | 0.134 | -2.508 | -1.76 | -72.74 |
| UCC | 332.322 | 60.352 | 0.123 | -2.506 | -1.761 | -72.742 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=3.2, m-M=13.3, logA=8.7 |
Search coordinates in Bayestar19