MWSC 5572
Summary
MWSC 5572 is a poorly populated, 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: 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) | 28.575 | -78.965 | – | 3.27 | -11.38 | – |
| Bica et al. (2019) | 28.556 | -78.967 | – | – | – | – |
| UCC | 28.736 | -78.962 | 0.015 | 1.284 | -1.224 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.187, distance=1472, log_age=9.3 |
Search coordinates in Bayestar19