CWNU 1252
Summary
CWNU 1252 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) | 41.178 | 60.513 | 1.181 | -0.206 | -1.362 | – |
| Hunt & Reffert (2023) | 41.117 | 60.536 | 1.177 | -0.265 | -1.254 | 2.143 |
| Cavallo et al. (2024) | 41.447 | 60.452 | 1.177 | – | – | – |
| UCC | 41.251 | 60.521 | 1.188 | -0.268 | -1.289 | -1.061 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2022) | A0=2.45, logAge=8.15 |
| Hunt & Reffert (2023) | AV50=1.429, diffAV50=0.587, MOD50=9.543, logAge50=8.122 |
| Cavallo et al. (2024) | AV50=1.26, dMod50=10.26, logAge50=9.11, [Fe/H]50=0.14 |
Search coordinates in Bayestar19
