Hogg 11
Summary
Hogg 11 is a sparse, loose object of intermediate C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It is rarely studied in the literature, with no articles listed in the last 13 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) | 167.904 | -60.4 | – | -0.65 | 6.58 | – |
| Kharchenko et al. (2012) | 167.903 | -60.39 | – | -3.67 | 3.19 | – |
| UCC | 167.967 | -60.372 | 0.384 | -6.006 | 1.548 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.32, Dist=2270.0, Age=7.08 |
| Kharchenko et al. (2012) | e_bv=0.354, distance=2554, log_age=6.99 |
Search coordinates in Bayestar19