Article: New astrophysics research from I. Ramirez and colleagues discussed.

In this recent study, researchers in Garching, Germany conducted a study "To explore the impact of surface inhomogeneities on stellar spectra, granulation models need to be computed. Ideally, the most fundamental characteristics of these models should be carefully tested before applying them to the study of more practical matters, such as the derivation of photospheric abundances."

"Our goal is to analyze the particular case of a K-dwarf. We construct a three-dimensional radiative-hydrodynamic model atmosphere of parameters T-eff = 4820 K, log g = 4.5, and solar chemical composition. Using this model and 3D spectrum synthesis, we computed a number of Fe I and Fe ...

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