Poster title: Dynamical of dust in circumbinary discs not coplanar

Poster abstract: Currently, observations of protoplanetary discs had shown amazing structures, both in gas as in dust 
(HL Tau, TW Hya, Elias 2-27). In this work, it is studied the dynamical and distribution of dust to different sizes (100μm-
1cm) in a binary system similar to HD142527. The circumbinary dust disc has azimuthal asymmetries on its structure 
that are hard to explain. The aim of this work is to prove that these structures can be created by an eccentric and 
misalignment binary system respect to the disc. Considering different orbital parameters we study the dynamical of the 
resulted disc by hydrodynamical simulations 3D (Phantom) of gas and dust. Given that the coupling of dust to gas 
depends on its size, we obtain different results for each size considered. Finally, we process these results for creating 
synthetic images like-telescope to different wavelengths that can be compared with observations.