Barkhatova 2
Summary
Barkhatova 2 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It is poorly studied in the literature, with no articles listed in the last 8 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 |
|---|---|---|---|---|---|---|
| Dias et al. (2002) | 325.908 | 51.071 | – | -0.53 | -1.46 | – |
| Kharchenko et al. (2012) | 325.917 | 51.07 | – | -2.2 | -3.53 | – |
| Loktin & Popova (2017) | 325.905 | 51.071 | – | -1.976 | -3.402 | – |
| UCC | 325.855 | 51.048 | 0.275 | -4.188 | -4.305 | -65.986 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.77, Dist=1676.0, Age=6.85 |
| Kharchenko et al. (2012) | e_bv=0.3, distance=1100, log_age=8.632 |
| Loktin & Popova (2017) | E(B-V)=0.691, Dist=1529, logt=6.85 |
Search coordinates in Bayestar19