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Improved opacities and pulsation stability in subluminous B and O stars
Authors:C. S. Jeffery   H. Saio
Affiliation:Armagh Observatory, College Hill, Armagh BT61 9DG;Astronomical Institute, School of Science, Tohoku University, Sendai 980-8578, Japan
Abstract:
Keywords:atomic processes    radiative transfer    stars: early-type    stars: horizontal branch    stars: interiors    stars: oscillations
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