FSR 1718
(MWSC 2432)
Summary
FSR 1718 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It is poorly studied in the literature, with no articles listed in the last 6 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) | 249.517 | -57.087 | – | – | – | – |
| Kharchenko et al. (2012) | 249.518 | -57.095 | – | -6.91 | -0.53 | – |
| Bica et al. (2019) | 249.519 | -57.088 | – | – | – | – |
| UCC | 249.53 | -57.101 | 0.247 | -4.505 | -7.256 | -90.235 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.125, distance=2466, log_age=9.5 |
Search coordinates in Bayestar19