Sco OB5
Summary
Sco OB5 is a moderately populated, very dense object of high C3 quality. It is located at a relatively close distance from the Sun, below the mid-plane. It is poorly studied in the literature.
This object shares a large percentage of members with a later reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Piskunov et al. (2007) | 268.129 | -38.644 | – | – | – | – |
| Piskunov et al. (2008) | 268.129 | -38.644 | – | – | – | – |
| He et al. (2023) | 268.137 | -38.728 | 0.804 | 2.884 | -1.796 | -17.98 |
| UCC | 268.109 | -38.704 | 0.817 | 2.902 | -1.812 | -14.824 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Piskunov et al. (2007) | E(B-V)=0.23, Dist=3310, logt=6.86, logM=5.043 |
| Piskunov et al. (2008) | E(B-V)=0.23, Dist=3310, logt=6.86, logM=5.77, logMA=5.658 |
| He et al. (2023) | A0=1.0, m-M=10.55, logA=7.2 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| Alessi 80B | 98.0 | 268.11 | -38.69 | 0.81 | 2.9 | -1.77 | -17.98 | 0.22 |