Theia 4432
Summary
Theia 4432 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 |
|---|---|---|---|---|---|---|
| Hunt & Reffert (2023) | 317.255 | 47.865 | 0.868 | -5.777 | -6.278 | -16.833 |
| Cavallo et al. (2024) | 317.504 | 47.997 | 0.869 | – | – | – |
| Hunt & Reffert (2024) | 317.255 | 47.865 | 0.868 | -5.777 | -6.278 | -16.833 |
| UCC | 317.46 | 47.933 | 0.877 | -5.765 | -6.316 | -15.368 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=1.4, diffAV50=0.512, MOD50=10.226, logAge50=8.076 |
| Cavallo et al. (2024) | AV50=1.5, dMod50=10.44, logAge50=8.38, [Fe/H]50=0.26 |
| Hunt & Reffert (2024) | MassJ=59.9934, MassTot=93.8123 |
Search coordinates in Bayestar19
