FSR 1293
Summary
FSR 1293 is a sparse, very loose object of very low C3 quality. It is located at a 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) | 110.983 | -25.36 | – | – | – | – |
| Kharchenko et al. (2012) | 110.984 | -25.359 | – | -0.77 | 4.71 | – |
| UCC | 110.93 | -25.394 | 0.17 | -1.079 | 1.357 | 63.653 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=1.197, distance=962, log_age=9.005 |
Search coordinates in Bayestar19