DBSB 79
Summary
DBSB 79 is a sparse, very loose object of low C3 quality. It is located at a very large distance from the Sun, below the mid-plane. It is rarely studied in the literature, with no articles listed in the last 13 years.
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. (2012) | 192.195 | -63.728 | – | -11.45 | 3.81 | – |
| UCC | 192.16 | -63.771 | 0.075 | -6.754 | -0.039 | -25.768 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=1.041, distance=1489, log_age=8.4 |
Search coordinates in Bayestar19