MWSC 4137
Summary
MWSC 4137 is a poorly populated, very loose object of low C3 quality. It is located at a 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: 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) | 141.548 | -79.74 | – | -4.09 | 8.78 | – |
| Bica et al. (2019) | 141.567 | -79.739 | – | – | – | – |
| UCC | 141.6 | -79.744 | 0.17 | -2.747 | 4.294 | 25.703 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.271, distance=1209, log_age=9.21 |
Search coordinates in Bayestar19