3D hydrodynamic simulations of carbon burning in massive stars

3D hydrodynamic simulations of carbon burning in massive stars

We present the first detailed 3D hydrodynamic implicit large eddy simulations of turbulent convection of carbon burning in massive stars. Simulations begin with radial profiles mapped from a carbon-burning shell within a 15M circle dot 1D stellar evolution model. We consider models with 128(3), 256(...

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Bibliographic Details
Main Authors: Cristini, A., Meakin, C., Hirschi, R., Arnett, D., Georgy, C., Viallet, M., Walkington, I.
Other Authors: Univ Arizona, Dept Astron
Language:en
Published: OXFORD UNIV PRESS 2017
Subjects:
convection
hydrodynamics
turbulence
stars: evolution
stars: interiors
stars: massive
Online Access:http://hdl.handle.net/10150/625735
http://arizona.openrepository.com/arizona/handle/10150/625735

Internet

http://hdl.handle.net/10150/625735
http://arizona.openrepository.com/arizona/handle/10150/625735

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