ADS 13292
Summary
ADS 13292 is a moderately populated, very dense object of high C3 quality. It is located at a relatively close distance from the Sun, above the mid-plane. It is rarely studied in the literature, with no articles listed in the last 19 years.
This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Kronberger et al. (2006) | 300.597 | 35.311 | – | – | – | – |
| UCC | 300.598 | 35.313 | 0.515 | -3.353 | -6.713 | -5.664 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kronberger et al. (2006) | E(B-V)=0.58, Dist=1.6, logt=7.0 |
Search coordinates in Bayestar19
Cluster region
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| Teutsch 8 | 24.1 | 300.61 | 35.31 | 0.51 | -3.39 | -6.72 | -10.86 | 0.7 |