FSR 1757
(MWSC 2869)
Summary
FSR 1757 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 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) | 274.267 | -45.257 | – | – | – | – |
| Kharchenko et al. (2012) | 274.26 | -45.25 | – | -0.29 | -1.58 | – |
| Bica et al. (2019) | 274.266 | -45.252 | – | – | – | – |
| UCC | 274.267 | -45.229 | 0.192 | -4.129 | -3.87 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.229, distance=1397, log_age=8.66 |
Search coordinates in Bayestar19