FSR 1709
Summary
FSR 1709 is a sparse, very loose object of intermediate C3 quality. It is located at a very large distance from the Sun, below the mid-plane. It is rarely studied in the literature, with no articles listed in the last 13 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 |
|---|---|---|---|---|---|---|
| Froebrich et al. (2007) | 239.392 | -54.363 | – | – | – | – |
| Kharchenko et al. (2012) | 239.37 | -54.375 | – | -0.64 | -1.0 | – |
| UCC | 239.382 | -54.38 | 0.086 | -4.953 | -4.407 | -97.775 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.666, distance=1893, log_age=8.5 |
Search coordinates in Bayestar19