Testing Lyα Emission-line Reconstruction Routines at Multiple Velocities in One System
Date Issued
2022-09
Author(s) USM
DOI
10.3847/1538-4357/ac87a8
Abstract
The 1215.67 angstrom H i Ly alpha emission line dominates the ultraviolet flux of low-mass stars, including the majority of known exoplanet hosts. Unfortunately, strong attenuation by the interstellar medium (ISM) obscures the line core in most stars, req
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