HST/STIS high-resolution NUV and FUV spectroscopy is essential and irreplaceable for constraining atmospheric structure and the onset of mass loss in evolved stars.
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The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars
HST/STIS high-resolution NUV and FUV spectroscopy is essential and irreplaceable for constraining atmospheric structure and the onset of mass loss in evolved stars.