CWNU 1974
Summary
CWNU 1974 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It was recently reported in the literature.
Warning: contains less than 25 stars with P>0.5 estimated.
Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicates that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| He et al. (2023) | 114.388 | -34.774 | 0.442 | -3.655 | 3.704 | – |
| Hunt & Reffert (2023) | 114.397 | -34.834 | 0.417 | -3.636 | 3.731 | – |
| Cavallo et al. (2024) | 114.356 | -34.746 | 0.42 | – | – | – |
| UCC | 114.358 | -34.769 | 0.43 | -3.655 | 3.75 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.75, m-M=11.75, logAge=7.3 |
| Hunt & Reffert (2023) | AV50=1.374, diffAV50=1.372, MOD50=11.675, logAge50=8.062 |
| Cavallo et al. (2024) | AV50=0.92, dMod50=11.5, logAge50=8.46, [Fe/H]50=0.02 |
Search coordinates in Bayestar19