MWSC 4211
Summary
MWSC 4211 is a sparse, very loose object of very low C3 quality. It is located at a moderate distance from the Sun, well above the mid-plane. It is rarely studied in the literature, with no articles listed in the last 6 years.
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 |
|---|---|---|---|---|---|---|
| Kharchenko et al. (2012) | 232.898 | -37.49 | – | -8.27 | -3.97 | – |
| Bica et al. (2019) | 232.9 | -37.484 | – | – | – | – |
| UCC | 232.888 | -37.448 | 0.382 | -7.231 | -1.992 | -58.096 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.729, distance=2361, log_age=8.82 |
Search coordinates in Bayestar19