CWNU 2259
Summary
CWNU 2259 is a sparse, very loose object of intermediate C3 quality. It is located at a moderate 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) | 111.021 | -18.349 | 0.316 | -2.387 | 2.97 | 64.21 |
| Hunt & Reffert (2023) | 110.802 | -18.634 | 0.319 | -2.427 | 3.003 | – |
| Cavallo et al. (2024) | 110.837 | -18.396 | 0.318 | – | – | – |
| UCC | 110.893 | -18.427 | 0.32 | -2.424 | 2.998 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.0, m-M=12.4, logAge=8.75 |
| Hunt & Reffert (2023) | AV50=0.775, diffAV50=0.958, MOD50=12.283, logAge50=8.194 |
| Cavallo et al. (2024) | AV50=1.11, dMod50=12.19, logAge50=7.93, [Fe/H]50=-0.32 |
Search coordinates in Bayestar19
