NGC 7394
Summary
NGC 7394 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It is rarely studied in the literature, with no articles listed in the last 8 years.
Warning: contains less than 25 stars with P>0.5 estimated.
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) | 342.596 | 52.135 | – | -1.41 | -0.6 | – |
| Loktin & Popova (2017) | 342.6 | 52.135 | – | -1.381 | -0.286 | – |
| UCC | 342.657 | 52.133 | 0.212 | -4.063 | -1.857 | -69.716 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.35, Dist=1310.0, Age=8.78 |
| Loktin & Popova (2017) | E(B-V)=0.183, Dist=2980, logt=8.59 |
Search coordinates in Bayestar19