MWSC 5295
Summary
MWSC 5295 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 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) | 233.662 | -13.38 | – | -4.26 | -4.5 | – |
| Kharchenko et al. (2016) | 233.655 | -13.379 | – | – | – | – |
| Bica et al. (2019) | 233.651 | -13.375 | – | – | – | – |
| Just et al. (2023) | 233.655 | -13.379 | – | – | – | – |
| UCC | 233.691 | -13.389 | 0.39 | -8.311 | -1.384 | -120.658 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Schmeja et al. (2014) | E(B-V)=0.208, d=1764.0, logt=9.36 |
| Kharchenko et al. (2016) | E(B-V)=0.208, d=1764.0, logt=9.36 |
| Just et al. (2023) | logt=9.36, logmt=2.686 |
Search coordinates in Bayestar19