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Constructing stable 3D hydrodynamical models of giant stars

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Hydrodynamical simulations of stellar interactions require stable models of stars as initial conditions. Such initial models, however, are difficult to construct for giant stars because of the wide range in spatial scales of the hydrostatic equilibrium and in dynamical timescales between the core an...

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Main Authors: Ohlmann, Sebastian T. (Author) , Röpke, Friedrich (Author) , Pakmor, Rüdiger (Author) , Springel, Volker (Author)
Format: Article (Journal)
Language:English
Published: 20 February 2017
In: Astronomy and astrophysics
Year: 2017, Volume: 599
ISSN:1432-0746
DOI:10.1051/0004-6361/201629692
Online Access:Verlag, kostenfrei, Volltext: http://dx.doi.org/10.1051/0004-6361/201629692
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Author Notes:Sebastian T. Ohlmann, Friedrich K. Röpke, Rüdiger Pakmor, and Volker Springel
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Constructing stable 3D hydrodynamical models of giant stars by Ohlmann, Sebastian T. (Author) , Röpke, Friedrich (Author) , Pakmor, Rüdiger (Author) , Springel, Volker (Author) ,


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