The role of convection in stellar models

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dc.contributor.author Moonsamy, Sashin
dc.date.accessioned 2011-07-21T12:49:32Z
dc.date.available 2011-07-21T12:49:32Z
dc.date.issued 2011-07-21
dc.identifier.uri http://hdl.handle.net/10539/10308
dc.description.abstract This thesis reviews the essential ingredients of local, time-independent mixing-length theory, the convective stability of uid elements in the stellar interior, the origins and in uence of convection zones in stars, and the numerical implementation of convection in some popular stellar evolution codes. The thesis concludes with a brief discussion of the future role of mixing-length theory in stellar modelling. en_US
dc.language.iso en en_US
dc.title The role of convection in stellar models en_US
dc.type Thesis en_US


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