LP 18
Summary
LP 18 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 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) | 79.155 | 32.614 | – | 2.948 | -6.962 | – |
| UCC | 79.206 | 32.581 | 0.247 | 0.497 | -0.36 | 1.778 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Loktin & Popova (2017) | E(B-V)=0.541, Dist=2419, logt=9.0 |
Search coordinates in Bayestar19