LP 42
Summary
LP 42 is a sparse, very loose object of very low C3 quality. It is located at a large distance from the Sun, below the mid-plane. It is rarely 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 |
|---|---|---|---|---|---|---|
| Loktin & Popova (2017) | 100.065 | 2.055 | – | 1.468 | -0.95 | – |
| UCC | 100.055 | 2.051 | 0.167 | -0.382 | 0.627 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Loktin & Popova (2017) | E(B-V)=0.688, Dist=3626, logt=6.6 |
Search coordinates in Bayestar19