A simulation-based line shape code that alternates between atomic and molecular bases yields broader quasi-H2+ satellites that better match a white dwarf's ultraviolet spectrum.
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A New Approach to Modeling Line Shapes with Quasi-H$_2^+$ Satellites in Stellar Atmospheres
A simulation-based line shape code that alternates between atomic and molecular bases yields broader quasi-H2+ satellites that better match a white dwarf's ultraviolet spectrum.