CWNU 2407
Summary
CWNU 2407 is a sparse, very loose object of low C3 quality. It is located at a relatively close 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) | 117.675 | -32.769 | 0.621 | -2.433 | 1.878 | – |
| Hunt & Reffert (2023) | 117.696 | -32.973 | 0.608 | -2.404 | 1.848 | -11.593 |
| Cavallo et al. (2024) | 117.672 | -32.7 | 0.611 | – | – | – |
| UCC | 117.704 | -32.737 | 0.62 | -2.404 | 1.864 | -11.473 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.75, m-M=10.95, logAge=7.55 |
| Hunt & Reffert (2023) | AV50=1.295, diffAV50=1.583, MOD50=10.932, logAge50=8.086 |
| Cavallo et al. (2024) | AV50=1.2, dMod50=11.17, logAge50=7.76, [Fe/H]50=0.52 |
Search coordinates in Bayestar19