CWNU 2015
Summary
CWNU 2015 is a poorly populated, very dense object of very 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) | 134.346 | -48.336 | 0.427 | -4.401 | 3.599 | – |
| Hunt & Reffert (2023) | 134.322 | -48.313 | 0.441 | -4.42 | 3.608 | – |
| Cavallo et al. (2024) | 134.359 | -48.34 | 0.439 | – | – | – |
| Hunt & Reffert (2024) | 134.322 | -48.313 | 0.441 | -4.42 | 3.608 | – |
| UCC | 134.339 | -48.348 | 0.427 | -4.456 | 3.602 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=3.55, m-M=12.1, logAge=6.15 |
| Hunt & Reffert (2023) | AV50=5.261, diffAV50=1.869, MOD50=11.719, logAge50=7.893 |
| Cavallo et al. (2024) | AV50=4.74, dMod50=12.42, logAge50=7.93, [Fe/H]50=0.5 |
| Hunt & Reffert (2024) | MassJ=385.372, MassTot=385.372 |
Search coordinates in Bayestar19
