A Semiempirical Estimate of Solar Extreme-ultraviolet Evolution from 10 Myr to 10 Gyr

A Semiempirical Estimate of Solar Extreme-ultraviolet Evolution from 10 Myr to 10 Gyr

The extreme-ultraviolet (EUV; 100–911 Å) spectra of F, G, K, and M stars provide diagnostics of the stellar chromosphere through the corona, with line and continuum formation temperatures spanning roughly 10 ^4 –10 ^7 K. The EUV stellar spectrum in turn drives atmospheric photochemistry and numerous...

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Bibliographic Details
Main Authors: Kevin France, Girish Duvvuri, Cynthia S. Froning, Alexander Brown, P. Christian Schneider, J. Sebastian Pineda, David Wilson, Allison Youngblood, Vladimir S. Airapetian, Kosuke Namekata, Yuta Notsu, Tristen Sextro
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astronomical Journal
Subjects:
Solar extreme ultraviolet emission
Stellar activity
Exoplanet atmospheres
Online Access:https://doi.org/10.3847/1538-3881/adefdf
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https://doi.org/10.3847/1538-3881/adefdf

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