CWNU 1824
Summary
CWNU 1824 is a poorly populated, very loose object of very 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: 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) | 94.691 | 4.407 | 0.725 | -1.105 | -1.797 | – |
| Hunt & Reffert (2023) | 94.465 | 4.362 | 0.725 | -1.11 | -1.789 | – |
| Cavallo et al. (2024) | 94.662 | 4.352 | 0.726 | – | – | – |
| Zhang et al. (2024) | 94.465 | 4.362 | – | – | – | – |
| UCC | 94.699 | 4.364 | 0.721 | -1.117 | -1.802 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=0.4, m-M=10.85, logAge=6.75 |
| Hunt & Reffert (2023) | AV50=1.594, diffAV50=1.34, MOD50=10.541, logAge50=8.445 |
| Cavallo et al. (2024) | AV50=1.99, dMod50=10.78, logAge50=7.96, [Fe/H]50=-0.19 |
| Zhang et al. (2024) | [Fe/H]ANN=-0.1415, [Fe/H]MCMC=-0.1135 |
Search coordinates in Bayestar19