3D AMR simulations of the evolution of the diffuse gas cloud G2 in the Galactic Centre

M. Schartmann , A. Ballone , A. Burkert , S. Gillessen , R. Genzel , O. Pfuhl , F. Eisenhauer , P.M. Plewa

show 3 more authors

T. Ott E.M. George M. Habibi

Authors on Pith no claims yet

classification 🌌 astro-ph.GA

keywords clouddiffuseevolutionsimulationscentrecomingdiscexploring

0 comments

read the original abstract

With the help of 3D AMR hydrodynamical simulations we aim at understanding G2's nature, recent evolution and fate in the coming years. By exploring the possible parameter space of the diffuse cloud scenario, we find that a starting point within the disc of young stars is favoured by the observations, which may hint at G2 being the result of stellar wind interactions.

This paper has not been read by Pith yet.

3D AMR simulations of the evolution of the diffuse gas cloud G2 in the Galactic Centre

discussion (0)