http://arxiv.org/abs/1609.07308
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.
M. Schartmann, A. Ballone, A. Burkert, et. al.
Mon, 26 Sep 16
14/48
Comments: Proceedings IAU Symposium No. 322, The Multi-Messenger Astrophysics of the Galactic Centre, 2016, S. Longmore, G. Bicknell & R. Crocker, eds
You must be logged in to post a comment.