FSR 1713
Summary
FSR 1713 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, well 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) | 251.2 | -58.856 | – | – | – | – |
| Kharchenko et al. (2012) | 251.215 | -58.86 | – | 1.12 | 1.96 | – |
| UCC | 251.267 | -58.891 | 0.189 | -3.161 | -4.304 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.104, distance=4935, log_age=9.3 |
Search coordinates in Bayestar19