MWSC 4116
Summary
MWSC 4116 is a sparse, very loose object of high 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) | 94.8 | -59.97 | – | -0.92 | 8.55 | – |
| Bica et al. (2019) | 94.795 | -59.968 | – | – | – | – |
| UCC | 94.749 | -59.984 | -0.03 | 1.556 | 0.657 | 312.721 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.291, distance=1743, log_age=9.125 |
Search coordinates in Bayestar19