MWSC 4355
Summary
MWSC 4355 is a sparse, very loose object of low C3 quality. It is located at a very large 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) | 262.65 | -23.935 | – | 1.43 | -3.73 | – |
| Bica et al. (2019) | 262.649 | -23.937 | – | – | – | – |
| UCC | 262.668 | -23.956 | 0.093 | -6.214 | -3.839 | -30.18 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=1.145, distance=1113, log_age=8.68 |
Search coordinates in Bayestar19