Radiation-hydrodynamical model atmospheres across the Hertzsprung-Russell diagram

Autores
Prof.
Hans-G. Ludwig
Fecha y hora
29 Abr 2008 - 00:00 Europe/London
Dirección

Aula

Idioma de la charla
Inglés
Idioma de la presentación
Inglés
Número en la serie
0
Descripción
In the EU funded Marie Curie Excellence Team CIFIST (Cosmological Impact of the FIrst STars) work is under way to construct 3D radiation-hydrodynamical model atmospheres for late-type dwarfs and giants, in particular of low metallicity. I will present an overview of the present state of the efforts, discuss some applications of the models, and point to necessary future developments.
Formato
Seminario
Vídeo de la charla
https://youtu.be/KiC7fiRFmUA
Estrellas tardías
Transferencia radiativa

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