The X-ray temperature-brightness relation of nearby FGK stars is explained by the RTV coronal-loop scaling law, with a nearly universal loop-length-to-filling-factor ratio.
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The X-ray catalogue of FGK stars within 10 pc: The coronal temperature-brightness relation explained with the RTV scaling law
The X-ray temperature-brightness relation of nearby FGK stars is explained by the RTV coronal-loop scaling law, with a nearly universal loop-length-to-filling-factor ratio.