DBSB 64
Summary
DBSB 64 is a sparse, loose object of low C3 quality. It is located at a close distance from the Sun, 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 |
|---|---|---|---|---|---|---|
| Kharchenko et al. (2012) | 171.143 | -58.95 | – | -10.86 | 2.03 | – |
| Hunt & Reffert (2023) | 170.973 | -58.92 | 1.073 | -10.502 | 2.07 | -21.983 |
| Cavallo et al. (2024) | 170.699 | -58.96 | 1.072 | – | – | – |
| UCC | 170.77 | -58.932 | 1.077 | -10.531 | 2.031 | -17.774 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.458, distance=5254, log_age=6.2 |
| Hunt & Reffert (2023) | AV50=0.129, diffAV50=0.793, MOD50=9.767, logAge50=8.016 |
| Cavallo et al. (2024) | AV50=0.28, dMod50=9.76, logAge50=8.11, [Fe/H]50=0.04 |
Search coordinates in Bayestar19
