MWSC 4429
Summary
MWSC 4429 is a sparse, very loose object of 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) | 278.895 | -51.745 | – | -0.46 | -5.08 | – |
| Bica et al. (2019) | 278.893 | -51.746 | – | – | – | – |
| UCC | 278.891 | -51.728 | 0.22 | -2.798 | -4.397 | -133.797 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.437, distance=2051, log_age=9.045 |
Search coordinates in Bayestar19