CWNU 1465
Summary
CWNU 1465 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.This is a unique object, which shares a very small percentage of members with at least one previously reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| He et al. (2023) | 270.362 | -23.532 | 0.358 | -0.44 | -1.626 | – |
| Hunt & Reffert (2023) | 270.365 | -23.546 | 0.346 | -0.42 | -1.61 | – |
| Cavallo et al. (2024) | 270.362 | -23.528 | 0.346 | – | – | – |
| Hunt & Reffert (2024) | 270.365 | -23.546 | 0.346 | -0.42 | -1.61 | – |
| UCC | 270.365 | -23.543 | 0.339 | -0.439 | -1.635 | 22.07 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=3.2, m-M=11.95, logAge=7.5 |
| Hunt & Reffert (2023) | AV50=2.985, diffAV50=1.436, MOD50=12.098, logAge50=7.182 |
| Cavallo et al. (2024) | AV50=3.31, dMod50=11.0, logAge50=7.74, [Fe/H]50=-0.59 |
| Hunt & Reffert (2024) | MassJ=541.294, MassTot=541.294 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| Ruprecht 139 | 2.3 | 270.23 | -23.53 | 0.32 | -0.01 | -1.41 | 1.35 | 0.73 |
