MWSC 4682
Summary
MWSC 4682 is a poorly populated, very loose object of very low C3 quality. It is located at a moderate distance from the Sun, well below the mid-plane. It is poorly studied in the literature.
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 |
|---|---|---|---|---|---|---|
| Scholz et al. (2015) | 355.845 | -82.96 | – | 5.87 | 0.28 | – |
| Kharchenko et al. (2016) | 355.847 | -82.963 | – | – | – | – |
| Bica et al. (2019) | 355.827 | -82.957 | – | – | – | – |
| Just et al. (2023) | 355.847 | -82.963 | – | – | – | – |
| UCC | 355.75 | -82.956 | 0.345 | 8.339 | -4.311 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Scholz et al. (2015) | E(B-V)=0.354, d=1065.0, logt=9.28 |
| Kharchenko et al. (2016) | E(B-V)=0.354, d=1065.0, logt=9.28 |
| Just et al. (2023) | logt=9.28, logmt=2.321 |
Search coordinates in Bayestar19