MWSC 4248
Summary
MWSC 4248 is a sparse, very loose object of very 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: 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) | 243.188 | -29.905 | – | -1.12 | -1.41 | – |
| Bica et al. (2019) | 243.185 | -29.904 | – | – | – | – |
| UCC | 243.149 | -29.942 | 0.298 | -7.679 | -3.384 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.791, distance=1618, log_age=8.9 |
Search coordinates in Bayestar19