CWNU 1499
Summary
CWNU 1499 is a poorly populated, very loose object of high 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: 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) | 290.671 | 2.851 | 0.793 | -0.978 | -2.093 | – |
| UCC | 290.642 | 2.767 | 0.793 | -0.984 | -2.104 | 30.614 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.6, m-M=10.45, logAge=7.75 |
Search coordinates in Bayestar19