FSR 0851
Summary
FSR 0851 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.
This object shares a small percentage of members with a later reported entry.
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) | 78.662 | 19.8 | – | – | – | – |
| Kharchenko et al. (2012) | 78.66 | 19.815 | – | 1.76 | -5.22 | – |
| UCC | 78.654 | 19.819 | 0.163 | 0.289 | -0.702 | -8.504 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.958, distance=1092, log_age=9.15 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| Cmg 38 | 16.0 | 78.78 | 19.94 | 0.19 | 0.28 | -1.08 | -1.3 | 0.03 |