MWSC 5051
Summary
MWSC 5051 is a sparse, very dense object of very low C3 quality. It is located at a relatively close 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) | 146.468 | -7.005 | – | -4.55 | -1.27 | – |
| Bica et al. (2019) | 146.466 | -7.0 | – | – | – | – |
| UCC | 146.461 | -6.962 | 0.949 | -11.505 | -1.377 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.229, distance=1365, log_age=9.45 |
Search coordinates in Bayestar19