Theia 411
Summary
Theia 411 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 |
|---|---|---|---|---|---|---|
| Hunt & Reffert (2023) | 155.234 | -60.684 | 1.434 | -9.83 | 6.31 | -2.751 |
| Cavallo et al. (2024) | 155.311 | -60.691 | 1.432 | – | – | – |
| Hu & Soubiran (2025) | 155.311 | -60.691 | – | – | – | – |
| UCC | 155.207 | -60.749 | 1.409 | -9.91 | 6.263 | 0.248 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.247, diffAV50=1.004, MOD50=9.111, logAge50=7.987 |
| Cavallo et al. (2024) | AV50=0.0, dMod50=9.27, logAge50=8.74, [Fe/H]50=0.71 |
| Hu & Soubiran (2025) | MA22=-0.26, MA23f=-0.15, MZ23=-0.27, MK24=-0.19, MF24=-0.12 |
Search coordinates in Bayestar19
