Inversions of Stellar Structure From Asteroseismic Data

The advent of space-based photometry missions in the early 21st century enabled application to asteroseismic data advanced inference techniques until then restricted field helioseismology. high quality observations, discovery mixed modes evolved solar-like oscillators and need for an improvement determination stellar fundamental parameters such as mass, radius age led development sophisticated modelling tools, amongst which seismic inversions play a key role. In this review, we will discuss existing inversion internal structure distant stars adapted from helio-to asteroseismology. We present results obtained various Kepler targets, their coupling other well limitations analyses perspectives future developments these approaches context current TESS PLATO mission, exploitation observed post-main sequence oscillators, variational formulations might not provide sufficient accuracy.