NGC 6773
Summary
NGC 6773 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) | 288.762 | 4.882 | – | -2.57 | -1.55 | – |
| Loktin & Popova (2017) | 288.765 | 4.882 | – | -2.955 | -2.588 | – |
| UCC | 288.743 | 4.881 | 0.223 | -1.702 | -4.484 | 44.28 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=1.16, Dist=2160.0, Age=8.0 |
| Loktin & Popova (2017) | E(B-V)=0.776, Dist=3869, logt=9.03 |
Search coordinates in Bayestar19