TURBULENT CHEMICAL DIFFUSION IN CONVECTIVELY BOUNDED CARBON FLAMES

TURBULENT CHEMICAL DIFFUSION IN CONVECTIVELY BOUNDED CARBON FLAMES

It has been proposed that mixing induced by convective overshoot can disrupt the inward propagation of carbon deflagrations in super-asymptotic giant branch stars. To test this theory, we study an idealized model of convectively bounded carbon flames with 3D hydrodynamic simulations of the Boussines...

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Bibliographic Details
Main Authors: Lecoanet, Daniel, Schwab, Josiah, Quataert, Eliot, Bildsten, Lars, Timmes, F. X., Vasil, Geoffrey M., Oishi, Jeffrey S., Brown, Benjamin P., Burns, Keaton James
Other Authors: Massachusetts Institute of Technology. Department of Physics
Format: Article
Language:en_US
Published: IOP Publishing 2017
Online Access:http://hdl.handle.net/1721.1/108572
https://orcid.org/0000-0003-4761-4766

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http://hdl.handle.net/1721.1/108572
https://orcid.org/0000-0003-4761-4766

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