Improvements to stellar structure models, based on a grid of 3D convection simulations - I. T(t) relations
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)
|Collections||ANU Research Publications|
|Source:||Monthly Notices of the Royal Astronomical Society|
|01_Trampedach_Improvements_to_stellar_2014.pdf||914.54 kB||Adobe PDF|
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