DBSB 51
(MWSC 1822)
Summary
DBSB 51 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It is rarely 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 |
|---|---|---|---|---|---|---|
| Kharchenko et al. (2013) | 158.257 | -59.615 | – | -8.02 | 1.61 | – |
| Kharchenko et al. (2016) | 158.25 | -59.611 | – | – | – | – |
| Just et al. (2023) | 158.25 | -59.611 | – | – | – | – |
| UCC | 158.31 | -59.604 | 0.28 | -6.199 | 2.929 | -11.221 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2013) | E(B-V)=0.874, d=3189.0, logt=7.0 |
| Kharchenko et al. (2016) | E(B-V)=0.874, d=3189.0, logt=7.0 |
| Just et al. (2023) | logt=7.0, logmt=2.608 |
Search coordinates in Bayestar19