MWSC 5022
Summary
MWSC 5022 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, well above the mid-plane. It is poorly studied in the literature.
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 |
|---|---|---|---|---|---|---|
| Schmeja et al. (2014) | 124.099 | 0.45 | – | 3.36 | -2.5 | – |
| Kharchenko et al. (2016) | 124.093 | 0.453 | – | – | – | – |
| Bica et al. (2019) | 124.092 | 0.451 | – | – | – | – |
| Just et al. (2023) | 124.093 | 0.453 | – | – | – | – |
| UCC | 124.114 | 0.489 | 0.249 | -1.932 | -0.392 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Schmeja et al. (2014) | E(B-V)=0.208, d=1308.0, logt=9.17 |
| Kharchenko et al. (2016) | E(B-V)=0.208, d=1308.0, logt=9.17 |
| Just et al. (2023) | logt=9.17, logmt=1.411 |
Search coordinates in Bayestar19