FSR 1727
Summary
FSR 1727 is a sparse, very loose object of intermediate C3 quality. It is located at a very 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) | 247.467 | -49.752 | – | – | – | – |
| Kharchenko et al. (2012) | 247.455 | -49.752 | – | -4.33 | -1.17 | – |
| UCC | 247.434 | -49.721 | 0.062 | -4.153 | -4.968 | -64.998 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.937, distance=1201, log_age=8.87 |
Search coordinates in Bayestar19