MWSC 4410
Summary
MWSC 4410 is a sparse, very loose object of low C3 quality. It is located at a 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: 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) | 274.26 | -53.69 | – | -4.64 | -6.57 | – |
| Bica et al. (2019) | 274.264 | -53.693 | – | – | – | – |
| UCC | 274.252 | -53.714 | 0.153 | -3.214 | -5.325 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.625, distance=2202, log_age=8.9 |
Search coordinates in Bayestar19