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Model Photospheres for Late‐Type Stars from the Inversion of High‐Resolution Spectroscopic Observations: Groombridge 1830 and ε Eridani

Model Photospheres for Late‐Type Stars from the Inversion of High‐Resolution Spectroscopic Observations: Groombridge 1830 and ε Eridani

An inversion technique to recover LTE one-dimensional model photospheres for late-type stars, which was previously applied to the Sun (Allende Prieto et al. 1998), is now employed to reconstruct, semi-empirically, the photospheres of cooler dwarfs: the metal-poor Gmb1830 and the active star of solar-metallicity Eps Eri. The model atmospheres we …