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Wolfgang Brandner et al 2024 AJ 168 282
Modeling suggests that the observed gaps in the stellar sequence of open clusters are the result of small-number statistics and other factors, not evidence of the radiative–convective boundary.

Eleanna Asvestari et al 2024 ApJ 971 45
A wide-reaching meta-analysis of coronal magnetic field models finds that all of models studied fail to reproduce the boundaries of coronal holes seen in extreme-ultraviolet images.
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