FSR 1195
Summary
FSR 1195 is a sparse, very loose object of intermediate 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) | 104.792 | -12.992 | – | – | – | – |
| Kharchenko et al. (2012) | 104.82 | -12.95 | – | 0.36 | 2.6 | – |
| UCC | 104.825 | -12.942 | 0.145 | -0.56 | 1.458 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.958, distance=3150, log_age=8.2 |
Search coordinates in Bayestar19