MWSC 4005
Summary
MWSC 4005 is a poorly populated, very loose object of very low C3 quality. It is located at a moderate distance from the Sun, well below the mid-plane. It is rarely studied in the literature, with no articles listed in the last 6 years.
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 |
|---|---|---|---|---|---|---|
| Kharchenko et al. (2012) | 2.865 | -85.48 | – | 9.31 | -1.47 | – |
| Bica et al. (2019) | 2.892 | -85.477 | – | – | – | – |
| UCC | 2.906 | -85.464 | 0.237 | 1.245 | -0.571 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.25, distance=1159, log_age=9.375 |
Search coordinates in Bayestar19