Loden 89
Summary
Loden 89 is a sparse, loose object of very 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 |
|---|---|---|---|---|---|---|
| Piskunov et al. (2008) | 157.298 | -56.78 | – | – | – | – |
| Kharchenko et al. (2012) | 157.327 | -56.78 | – | -7.28 | 3.9 | – |
| Loktin & Popova (2017) | 157.305 | -56.783 | – | -6.05 | -0.48 | 20.05 |
| UCC | 157.327 | -56.796 | 0.268 | -6.125 | 3.264 | 17.997 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Piskunov et al. (2008) | E(B-V)=0.05, Dist=380, logt=8.47, logMA=1.551 |
| Kharchenko et al. (2012) | e_bv=0.05, distance=626, log_age=8.3 |
| Loktin & Popova (2017) | E(B-V)=0.05, Dist=366, logt=8.47 |
Search coordinates in Bayestar19