DBSB 88
Summary
DBSB 88 is a sparse, very loose object of high C3 quality. It is located at a 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) | 214.905 | -65.432 | – | -8.43 | -3.72 | – |
| UCC | 215.02 | -65.434 | 0.16 | -6.695 | -2.965 | -65.108 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=1.874, distance=1366, log_age=7.85 |
Search coordinates in Bayestar19