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Improvements to stellar structure models, based on a grid of 3D convection simulations - I. T(t) relations

Trampedach, Regner; Stein, R. F.; Christensen-Dalsgaard, J; Nordlund, A; Asplund, Martin

Description

Relations between temperature, T, and optical depth, τ, are often used for describing the photospheric transition from optically thick to optically thin in stellar structure models. We show that this is well justified, but also that currently used T(τ)

CollectionsANU Research Publications
Date published: 2014
Type: Journal article
URI: http://hdl.handle.net/1885/73832
Source: Monthly Notices of the Royal Astronomical Society
DOI: 10.1093/mnras/stu889

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