CWNU 2652
Summary
CWNU 2652 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, well below the mid-plane. It was recently reported in the literature.
Warning: contains less than 25 stars with P>0.5 estimated.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| He et al. (2023) | 89.343 | 11.217 | 0.213 | 0.262 | -0.178 | 36.96 |
| Hunt & Reffert (2023) | 89.337 | 11.332 | 0.178 | 0.272 | -0.256 | 38.543 |
| Cavallo et al. (2024) | 89.332 | 11.331 | 0.177 | – | – | – |
| Hunt & Reffert (2024) | 89.337 | 11.332 | 0.178 | 0.272 | -0.256 | 38.543 |
| UCC | 89.32 | 11.316 | 0.172 | 0.25 | -0.276 | 46.095 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=0.95, m-M=14.1, logAge=9.0 |
| Hunt & Reffert (2023) | AV50=0.316, diffAV50=1.918, MOD50=13.433, logAge50=8.96 |
| Cavallo et al. (2024) | AV50=0.46, dMod50=12.85, logAge50=9.01, [Fe/H]50=-0.58 |
| Hunt & Reffert (2024) | MassJ=233.197, MassTot=220.662 |
Search coordinates in Bayestar19
