NGC 6625
Summary
NGC 6625 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, above the mid-plane. It is poorly 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) | 275.708 | -11.962 | – | -0.71 | -1.21 | – |
| Kharchenko et al. (2012) | 275.697 | -11.955 | – | -1.72 | -3.43 | – |
| Loktin & Popova (2017) | 275.715 | -11.962 | – | -2.17 | -7.344 | – |
| UCC | 275.685 | -11.97 | 0.213 | -1.567 | -2.375 | -1.104 |
Estimated members
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Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=1.21, Dist=1335.0, Age=8.7 |
| Kharchenko et al. (2012) | e_bv=1.21, distance=1335, log_age=8.7 |
| Loktin & Popova (2017) | E(B-V)=0.145, Dist=1350, logt=8.95 |
Search coordinates in Bayestar19