High-resolution NUV and FUV spectroscopy from HST/STIS is uniquely capable of probing the atmospheric structure, chromospheres, and mass loss in evolved stars, and is essential for stellar astrophysics.
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The unique capabilities of HST for stellar physics Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars
High-resolution NUV and FUV spectroscopy from HST/STIS is uniquely capable of probing the atmospheric structure, chromospheres, and mass loss in evolved stars, and is essential for stellar astrophysics.