CWNU 313
Summary
CWNU 313 is a sparse, very loose object of very low C3 quality. It is located at a close distance from the Sun, below 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) | 294.705 | -1.134 | 1.65 | 0.36 | -2.48 | – |
| Hunt & Reffert (2023) | 295.138 | -1.992 | 1.722 | 0.556 | -2.529 | -15.903 |
| Cavallo et al. (2024) | 295.329 | -0.681 | 1.725 | – | – | – |
| UCC | 294.957 | -1.468 | 1.687 | 0.377 | -2.533 | -14.581 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2022) | AG=0.45, m-M=8.65, logAge=7.7, Z=0.026 |
| Hunt & Reffert (2023) | AV50=0.66, diffAV50=0.665, MOD50=8.71, logAge50=7.598 |
| Cavallo et al. (2024) | AV50=1.0, dMod50=8.97, logAge50=7.49, [Fe/H]50=0.26 |
Search coordinates in Bayestar19