Skip navigation
Skip navigation

Three-dimensional models of metal-poor stars

Collet, Remo


I present here the main results of recent realistic, three-dimensional (3D), hydrodynamical simulations of convection at the surface of metal-poor red giant stars. I discuss the application of these convection simulations as time-dependent, 3D, hydrodynamical model atmospheres to spectral line formation calculations and abundance analyses. The impact of 3D models on derived elemental abundances is investigated by means of a differential comparison of the line strengths predicted in 3D under the...[Show more]

CollectionsANU Research Publications
Date published: 2008
Type: Conference paper
Source: Physica Scripta, Volume T133
DOI: 10.1088/0031-8949/2008/T133/014004


File Description SizeFormat Image
01_Collet_Three-dimensional_models_of_2008.pdf3.04 MBAdobe PDF    Request a copy

Items in Open Research are protected by copyright, with all rights reserved, unless otherwise indicated.

Updated:  20 July 2017/ Responsible Officer:  University Librarian/ Page Contact:  Library Systems & Web Coordinator