MWSC 4225
Summary
MWSC 4225 is a sparse, loose 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) | 237.075 | -18.305 | – | -3.58 | -5.79 | – |
| Bica et al. (2019) | 237.078 | -18.303 | – | – | – | – |
| UCC | 237.073 | -18.328 | 0.522 | -6.32 | -3.789 | -18.917 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.822, distance=2495, log_age=8.7 |
Search coordinates in Bayestar19