Pages that link to "Item:Q1716130"
From MaRDI portal
The following pages link to Asymptotic orbits in Hill's problem when the larger primary is a source of radiation (Q1716130):
Displaying 2 items.
- Numerical determination of homoclinic and heteroclinic orbits at collinear equilibria in the restricted three-body problem with oblateness (Q819166) (← links)
- On the stability of the triangular equilibrium points in the photogravitational R3BP with an oblate infinitesimal and triaxial primaries for the binary lalande 21258 system (Q2080481) (← links)