CWNU 1954
Summary
CWNU 1954 is a poorly populated, very dense object of very high C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It was recently reported in the literature.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| He et al. (2023) | 248.25 | -48.574 | 0.334 | -3.327 | -3.741 | -69.14 |
| Hunt & Reffert (2023) | 248.249 | -48.585 | 0.296 | -3.311 | -3.701 | -52.657 |
| Cavallo et al. (2024) | 248.228 | -48.597 | 0.296 | – | – | – |
| Hunt & Reffert (2024) | 248.249 | -48.585 | 0.296 | -3.311 | -3.701 | -52.657 |
| UCC | 248.236 | -48.586 | 0.308 | -3.33 | -3.74 | -69.144 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=5.1, m-M=12.05, logAge=8.55 |
| Hunt & Reffert (2023) | AV50=3.411, diffAV50=2.71, MOD50=12.375, logAge50=9.456 |
| Cavallo et al. (2024) | AV50=4.85, dMod50=12.92, logAge50=7.77, [Fe/H]50=-0.06 |
| Hunt & Reffert (2024) | MassJ=634.092, MassTot=543.583 |
Search coordinates in Bayestar19
