FSR 1076
(MWSC 1145)
Summary
FSR 1076 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, well above the mid-plane. It is poorly studied in the literature.
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) | 108.379 | 3.149 | – | – | – | – |
| Kharchenko et al. (2013) | 108.36 | 3.148 | – | -3.6 | 0.31 | – |
| Kharchenko et al. (2016) | 108.353 | 3.15 | – | – | – | – |
| Bica et al. (2019) | 108.384 | 3.149 | – | – | – | – |
| Just et al. (2023) | 108.353 | 3.15 | – | – | – | – |
| UCC | 108.343 | 3.134 | 0.156 | -0.669 | -0.551 | 79.141 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2013) | E(B-V)=0.416, d=1031.0, logt=8.96 |
| Kharchenko et al. (2016) | E(B-V)=0.416, d=1031.0, logt=8.96 |
| Just et al. (2023) | logt=8.96, logmt=1.331 |
Search coordinates in Bayestar19