FSR 1350
Summary
FSR 1350 is a poorly populated, very loose object of intermediate C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It is rarely studied in the literature, with no articles listed in the last 13 years.
This object shares a very small percentage of members with at least one entry reported in the same catalogue.
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) | 116.95 | -34.036 | – | – | – | – |
| Kharchenko et al. (2012) | 116.951 | -34.036 | – | -5.43 | 5.89 | – |
| UCC | 116.932 | -34.041 | 0.285 | -2.068 | 3.063 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.833, distance=1608, log_age=8.6 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| FSR 1347 | 3.1 | 117.03 | -33.71 | 0.26 | -2.15 | 3.12 | 110.58 | 0.78 |