MWSC 4114
Summary
MWSC 4114 is a sparse, very loose object of intermediate C3 quality. It is located at a very large 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: 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) | 91.965 | -78.22 | – | 0.23 | 5.86 | – |
| Bica et al. (2019) | 91.976 | -78.224 | – | – | – | – |
| UCC | 91.834 | -78.232 | 0.048 | 1.875 | 0.928 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.26, distance=962, log_age=9.4 |
Search coordinates in Bayestar19