CWNU 2157
Summary
CWNU 2157 is a sparse, very loose object of low C3 quality. It is located at a relatively 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. (2023) | 91.955 | 21.037 | 0.547 | 1.42 | -2.435 | 61.28 |
| Hunt & Reffert (2023) | 91.916 | 21.025 | 0.549 | 1.447 | -2.418 | – |
| Cavallo et al. (2024) | 92.107 | 21.031 | 0.551 | – | – | – |
| UCC | 91.959 | 21.01 | 0.547 | 1.426 | -2.42 | 61.28 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.4, m-M=11.4, logAge=6.95 |
| Hunt & Reffert (2023) | AV50=0.983, diffAV50=0.545, MOD50=11.133, logAge50=7.796 |
| Cavallo et al. (2024) | AV50=1.26, dMod50=11.38, logAge50=8.65, [Fe/H]50=-0.12 |
Search coordinates in Bayestar19
