Basel 6
Summary
Basel 6 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, above 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) | 301.7 | 38.35 | – | -2.21 | -2.99 | – |
| Kharchenko et al. (2012) | 301.673 | 38.365 | – | -5.17 | -1.98 | – |
| Loktin & Popova (2017) | 301.695 | 38.35 | – | -1.51 | -0.717 | – |
| UCC | 301.683 | 38.371 | 0.123 | -3.166 | -5.315 | -54.19 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.58, Dist=1548.0, Age=7.977 |
| Kharchenko et al. (2012) | e_bv=0.583, distance=3108, log_age=9.11 |
| Loktin & Popova (2017) | E(B-V)=0.575, Dist=1613, logt=8.071 |
Search coordinates in Bayestar19