FSR 1027
(MWSC 593)
Summary
FSR 1027 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 poorly studied in the literature, with no articles listed in the last 6 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) | 84.071 | -3.271 | – | – | – | – |
| Kharchenko et al. (2012) | 84.078 | -3.28 | – | -4.07 | 3.23 | – |
| Bica et al. (2019) | 84.071 | -3.269 | – | – | – | – |
| UCC | 84.1 | -3.279 | 0.11 | 0.245 | -0.114 | 58.235 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.521, distance=2325, log_age=9.11 |
Search coordinates in Bayestar19