Gulliver 41
Summary
Gulliver 41 is a moderately populated, very dense object of high C3 quality. It is located at a large distance from the Sun, below the mid-plane. It is rarely studied in the literature.This is a unique object, which shares a very small percentage of members with at least one previously reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Cantat-Gaudin et al. (2018) | 277.718 | -12.429 | 0.171 | -1.79 | -4.709 | – |
| Cantat-Gaudin et al. (2020) | 277.718 | -12.429 | 0.171 | -1.79 | -4.709 | – |
| UCC | 277.716 | -12.427 | 0.181 | -1.703 | -4.771 | 58.103 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Cantat-Gaudin et al. (2018) | dmode=5000.2 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| Ruprecht 141 | 2.5 | 277.82 | -12.33 | 0.33 | -1.47 | -4.25 | 20.69 | 0.23 |
