CWNU 2417
Summary
CWNU 2417 is a poorly populated, loose object of high C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It was recently reported in the literature.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| He et al. (2023) | 236.355 | -58.244 | 0.373 | -3.595 | -4.287 | -62.7 |
| Hunt & Reffert (2023) | 236.401 | -58.241 | 0.367 | -3.576 | -4.271 | -51.908 |
| Cavallo et al. (2024) | 236.41 | -58.233 | 0.369 | – | – | – |
| Hunt & Reffert (2024) | 236.401 | -58.241 | 0.367 | -3.576 | -4.271 | -51.908 |
| UCC | 236.393 | -58.228 | 0.373 | -3.591 | -4.293 | -62.702 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.6, m-M=11.9, logAge=8.85 |
| Hunt & Reffert (2023) | AV50=1.602, diffAV50=0.565, MOD50=11.971, logAge50=8.419 |
| Cavallo et al. (2024) | AV50=1.9, dMod50=11.9, logAge50=8.37, [Fe/H]50=0.16 |
| Hunt & Reffert (2024) | MassJ=178.955, MassTot=202.947 |
Search coordinates in Bayestar19
