FSR 1776
Summary
FSR 1776 is a sparse, very loose object of low C3 quality. It is located at a very 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) | 268.546 | -36.148 | – | – | – | – |
| Kharchenko et al. (2012) | 268.5 | -36.145 | – | -9.45 | -3.47 | – |
| UCC | 268.519 | -36.203 | 0.045 | -3.728 | -6.702 | -115.88 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.458, distance=8923, log_age=9.5 |
Search coordinates in Bayestar19