Mixing length theory - PowerPoint PPT Presentation

Flux Transport by Convection in Late-Type Stars (Mihalas 7.3)

Flux Transport by Convection in Late-Type Stars (Mihalas 7.3) . Schwarzschild Criterion Mixing Length Theory Convective Flux in Cool Star. Schwarzschild Stability Criterion. Does it occur? If will continue to rise → unstable If will sink again → stable. Δ r. bubble.

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A tool to simulate COROT light-curves

A tool to simulate COROT light-curves. R. Samadi 1 &amp; F. Baudin 2 1 : LESIA, Observatory of Paris/Meudon 2 : IAS, Orsay. Purpose : to provide a tool to simulate CoRoT light-curves of the seismology channel. Interests : To help the preparation of the scientific analyses

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