FSR 1775
(MWSC 2750)
Summary
FSR 1775 is a sparse, very loose object of intermediate 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) | 269.05 | -36.571 | – | – | – | – |
| Kharchenko et al. (2012) | 269.033 | -36.565 | – | -9.53 | -1.0 | – |
| Bica et al. (2019) | 269.047 | -36.573 | – | – | – | – |
| UCC | 269.007 | -36.59 | 0.107 | -3.169 | -6.682 | -74.016 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.468, distance=8508, log_age=9.6 |
Search coordinates in Bayestar19