CWNU 1216
Summary
CWNU 1216 is a sparse, very loose object of very low C3 quality. It is located at a very 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) | 316.79 | 47.054 | 3.46 | 8.4 | 0.582 | – |
| Hunt & Reffert (2023) | 316.614 | 47.186 | 3.419 | 9.292 | 3.487 | -21.123 |
| Cavallo et al. (2024) | 317.365 | 47.611 | 3.42 | – | – | – |
| UCC | 317.079 | 47.121 | 3.281 | 8.901 | 2.385 | -21.519 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2022) | A0=0.75, logAge=7.55 |
| Hunt & Reffert (2023) | AV50=0.014, diffAV50=0.236, MOD50=7.283, logAge50=8.259 |
| Cavallo et al. (2024) | AV50=0.7, dMod50=7.36, logAge50=7.33, [Fe/H]50=0.06 |
Search coordinates in Bayestar19
