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3D AMR simulations of the evolution of the diffuse gas cloud G2 in the Galactic Centre
Published online by Cambridge University Press: 09 February 2017
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.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 11 , Symposium S322: The Multi-Messenger Astrophysics of the Galactic Centre , July 2016 , pp. 241 - 242
- Copyright
- Copyright © International Astronomical Union 2017