NGC 6596
Summary
NGC 6596 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, near 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.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dias et al. (2002) | 274.387 | -16.65 | – | 1.31 | -1.32 | 128.84 |
| Piskunov et al. (2008) | 274.376 | -16.652 | – | – | – | – |
| Kharchenko et al. (2012) | 274.38 | -16.65 | – | 2.67 | -2.02 | – |
| Loktin & Popova (2017) | 274.395 | -16.65 | – | 2.361 | -3.406 | 128.84 |
| UCC | 274.301 | -16.66 | 0.368 | -0.449 | -2.592 | -21.034 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.15, Dist=1100.0, Age=8.6 |
| Piskunov et al. (2008) | E(B-V)=0.15, Dist=1100, logt=8.6, logMA=2.559 |
| Kharchenko et al. (2012) | e_bv=0.167, distance=932, log_age=8.6 |
| Loktin & Popova (2017) | E(B-V)=0.282, Dist=1597, logt=8.39 |
Search coordinates in Bayestar19