How stars shine: Infrared observations expose gaps in models of how stars distribute their light

Astronomers using Georgia State University's CHARA Array have discovered that nearby stars darken more significantly toward their edges at near-infrared wavelengths than predicted by existing models. This finding provides a new benchmark for understanding stellar structure and atmospheres.

Sources

• Phys.org — How stars shine: Infrared observations expose gaps in models of how stars distribute their light

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