Hogg 14
Summary
Hogg 14 is a sparse, very loose object of very low C3 quality. It is located at a moderate 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) | 187.15 | -59.817 | – | -9.22 | 1.08 | – |
| Kharchenko et al. (2012) | 187.185 | -59.81 | – | -9.48 | -4.0 | – |
| Loktin & Popova (2017) | 187.155 | -59.817 | – | -12.067 | -5.766 | – |
| UCC | 187.208 | -59.837 | 0.257 | -7.812 | 0.376 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.229, Dist=969.0, Age=8.099 |
| Kharchenko et al. (2012) | e_bv=0.229, distance=1036, log_age=8.1 |
| Loktin & Popova (2017) | E(B-V)=0.258, Dist=1342, logt=8.035 |
Search coordinates in Bayestar19