NGC 6595
Summary
NGC 6595 is a sparse, loose object of very low C3 quality. It is located at a relatively close distance from the Sun, near the mid-plane. It is rarely studied in the literature, with no articles listed in the last 23 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) | 274.267 | -19.865 | – | 2.73 | -3.26 | – |
| UCC | 274.252 | -19.927 | 0.665 | 2.561 | -3.046 | 25.047 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.94, Dist=1640.0, Age=8.65 |
Search coordinates in Bayestar19