MWSC 4289
Summary
MWSC 4289 is a sparse, very loose object of low C3 quality. It is located at a 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) | 251.52 | -20.94 | – | -0.76 | -0.95 | – |
| Bica et al. (2019) | 251.518 | -20.935 | – | – | – | – |
| UCC | 251.496 | -20.921 | 0.174 | -4.62 | -4.188 | 57.534 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.947, distance=2183, log_age=9.325 |
Search coordinates in Bayestar19