DBSB 100
(MWSC 2387)
Summary
DBSB 100 is a rich, very dense object of very high C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It is poorly studied in the literature.
This object shares a moderate percentage of members with a later reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Kharchenko et al. (2013) | 245.109 | -50.907 | – | -4.87 | -2.74 | – |
| Kharchenko et al. (2016) | 245.097 | -50.906 | – | – | – | – |
| Cantat-Gaudin et al. (2018) | 245.106 | -50.902 | 0.148 | -2.94 | -3.622 | – |
| Cantat-Gaudin et al. (2020) | 245.106 | -50.902 | 0.148 | -2.94 | -3.622 | – |
| Just et al. (2023) | 245.097 | -50.906 | – | – | – | – |
| UCC | 245.113 | -50.912 | 0.207 | -2.961 | -3.685 | -17.679 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2013) | E(B-V)=1.083, d=2240.0, logt=8.55 |
| Kharchenko et al. (2016) | E(B-V)=1.083, d=2240.0, logt=8.55 |
| Cantat-Gaudin et al. (2018) | dmode=5652.8 |
| Just et al. (2023) | logt=8.55, logmt=1.274 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| HSC 2761 | 27.4 | 245.3 | -50.94 | 0.24 | -3.01 | -3.84 | -29.69 | 0.38 |
