LP 17
Summary
LP 17 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 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) | 78.21 | 47.921 | – | -3.085 | -5.551 | – |
| UCC | 78.196 | 47.916 | 0.29 | 0.348 | -1.989 | -28.688 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Loktin & Popova (2017) | E(B-V)=0.38, Dist=2495, logt=6.8 |
Search coordinates in Bayestar19