NGC 7772
Summary
NGC 7772 is a poorly populated, very loose object of 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 8 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) | 357.942 | 16.247 | – | 12.29 | -9.5 | -24.0 |
| Kharchenko et al. (2012) | 357.942 | 16.245 | – | 12.29 | -9.5 | – |
| Loktin & Popova (2017) | 357.945 | 16.247 | – | 12.29 | -9.5 | -31.5 |
| UCC | 357.922 | 16.233 | 0.253 | 0.747 | -3.064 | -13.463 |
Estimated members
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Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.03, Dist=1500.0, Age=9.17 |
| Kharchenko et al. (2012) | e_bv=0.45, distance=1250, log_age=9.162 |
| Loktin & Popova (2017) | E(B-V)=0.01, Dist=595, logt=9.261 |
Search coordinates in Bayestar19