FSR 1327
Summary
FSR 1327 is a sparse, very loose object of very 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.
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) | 114.85 | -31.753 | – | – | – | – |
| Kharchenko et al. (2012) | 114.832 | -31.74 | – | -2.58 | 2.75 | – |
| UCC | 114.85 | -31.779 | 0.135 | -1.026 | 1.999 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.708, distance=2597, log_age=8.51 |
Search coordinates in Bayestar19