MWSC 5299
Summary
MWSC 5299 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) | 235.47 | -29.0 | – | -2.27 | -4.16 | – |
| Kharchenko et al. (2016) | 235.461 | -28.999 | – | – | – | – |
| Bica et al. (2019) | 235.467 | -29.0 | – | – | – | – |
| Just et al. (2023) | 235.461 | -28.999 | – | – | – | – |
| UCC | 235.464 | -29.015 | 0.296 | -5.188 | -5.596 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Schmeja et al. (2014) | E(B-V)=0.146, d=4473.0, logt=9.4 |
| Kharchenko et al. (2016) | E(B-V)=0.146, d=4473.0, logt=9.4 |
| Just et al. (2023) | logt=9.4, logmt=3.692 |
Search coordinates in Bayestar19