
Show Notes
New astronomical research is challenging our understanding of both stellar atmospheres and the origins of the Milky Way.
Observations from the CHARA Array show that nearby stars fade toward their edges more strongly in infrared light than current models predict, potentially affecting how astronomers measure stars and exoplanets.
Meanwhile, the MEGATRON simulations are revealing how the first generations of stars and galaxies may have shaped the Milky Way’s early history, incorporating the effects of Population III stars and supernovae.
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