NGC 7193
Summary
NGC 7193 is a poorly populated, loose object of very low C3 quality. It is located at a moderate distance from the Sun, well below the mid-plane. It is poorly studied in the literature, with no articles listed in the last 6 years.
Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicates that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dias et al. (2002) | 330.762 | 10.802 | – | -1.07 | -5.41 | – |
| Loktin & Popova (2017) | 330.765 | 10.802 | – | 0.122 | -1.745 | – |
| Angelo et al. (2019) | 330.783 | 10.804 | – | – | – | – |
| UCC | 330.741 | 10.806 | 0.436 | 2.533 | -3.634 | -70.079 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.03, Dist=1080.0, Age=9.65 |
| Loktin & Popova (2017) | E(B-V)=0.202, Dist=2265, logt=9.25 |
| Angelo et al. (2019) | dsun=1.25, Age=4.47, Mphot=11 |
Search coordinates in Bayestar19