CWNU 418
Summary
CWNU 418 is a sparse, very loose object of low C3 quality. It is located at a close distance from the Sun, near 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. (2022) | 96.387 | 8.43 | 1.06 | -1.25 | -3.85 | 34.1 |
| Hunt & Reffert (2023) | 96.358 | 8.382 | 1.093 | -1.261 | -3.886 | 14.044 |
| Cavallo et al. (2024) | 96.247 | 8.203 | 1.097 | – | – | – |
| UCC | 96.352 | 8.329 | 1.092 | -1.25 | -3.847 | 21.885 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2022) | AG=0.1, m-M=11.05, logAge=6.2, Z=0.002 |
| Hunt & Reffert (2023) | AV50=0.199, diffAV50=0.792, MOD50=9.666, logAge50=8.554 |
| Cavallo et al. (2024) | AV50=0.55, dMod50=9.77, logAge50=8.05, [Fe/H]50=0.07 |
Search coordinates in Bayestar19