CWNU 1962
Summary
CWNU 1962 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, near 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) | 108.47 | -10.52 | 0.332 | -0.563 | 0.213 | 58.64 |
| Hunt & Reffert (2023) | 108.477 | -10.52 | 0.336 | -0.587 | 0.215 | – |
| Hunt & Reffert (2024) | 108.477 | -10.52 | 0.336 | -0.587 | 0.215 | – |
| UCC | 108.459 | -10.524 | 0.33 | -0.575 | 0.213 | 58.642 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.5, m-M=12.5, logAge=8.8 |
| Hunt & Reffert (2023) | AV50=1.184, diffAV50=0.512, MOD50=12.265, logAge50=8.657 |
| Hunt & Reffert (2024) | MassJ=204.019, MassTot=204.019 |
Search coordinates in Bayestar19
