DBSB 70
Summary
DBSB 70 is a sparse, very dense object of intermediate C3 quality. It is located at a relatively close distance from the Sun, near the mid-plane. It is poorly studied in the literature.
This object shares a large percentage of members with a later reported entry.
Warning: contains less than 25 stars with P>0.5 estimated.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Kharchenko et al. (2012) | 177.135 | -62.285 | – | -7.65 | -2.9 | – |
| Hunt & Reffert (2023) | 177.13 | -62.317 | 0.923 | -8.321 | 0.949 | -6.259 |
| Cavallo et al. (2024) | 177.108 | -62.335 | 0.936 | – | – | – |
| Hunt & Reffert (2024) | 177.13 | -62.317 | 0.923 | -8.321 | 0.949 | -6.259 |
| UCC | 177.086 | -62.324 | 0.93 | -8.361 | 0.878 | -5.669 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.541, distance=1274, log_age=7.7 |
| Hunt & Reffert (2023) | AV50=0.786, diffAV50=1.144, MOD50=10.023, logAge50=7.687 |
| Cavallo et al. (2024) | AV50=0.96, dMod50=10.18, logAge50=7.4, [Fe/H]50=-0.13 |
| Hunt & Reffert (2024) | MassJ=52.3556, MassTot=73.3906 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWNU 1238 | 84.0 | 177.11 | -62.34 | 0.94 | -8.37 | 0.84 | -5.67 | 0.07 |
