MWSC 4486
Summary
MWSC 4486 is a sparse, very loose object of very low C3 quality. It is located at a moderate 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) | 291.0 | -60.725 | – | 5.19 | -7.74 | – |
| Bica et al. (2019) | 291.008 | -60.721 | – | – | – | – |
| UCC | 290.94 | -60.706 | 0.214 | -0.963 | -5.379 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.187, distance=2228, log_age=9.3 |
Search coordinates in Bayestar19