MWSC 4131
Summary
MWSC 4131 is a poorly populated, very loose object of intermediate C3 quality. It is located at a very large 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: 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) | 124.823 | 42.035 | – | -1.05 | -7.67 | – |
| Bica et al. (2019) | 124.82 | 42.033 | – | – | – | – |
| UCC | 124.828 | 42.05 | 0.046 | 0.166 | -0.629 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.083, distance=1058, log_age=9.4 |
Search coordinates in Bayestar19