MWSC 4290
Summary
MWSC 4290 is a poorly populated, very loose object of low C3 quality. It is located at a moderate 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: 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) | 251.655 | -9.195 | – | -3.09 | -5.28 | – |
| Bica et al. (2019) | 251.652 | -9.193 | – | – | – | – |
| UCC | 251.714 | -9.189 | 0.218 | -1.772 | -2.4 | 54.927 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=1.249, distance=2628, log_age=8.38 |
Search coordinates in Bayestar19