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Spectroscopy of Rapidly Oscillating Ap Stars
Published online by Cambridge University Press: 12 April 2016
Abstract
We identify Spectroscopic differences between roAp stars and Ap stars with no observational evidence for pulsation, but with otherwise similar Teff and log g values. These differences concern the abundance pattern, Hydrogen line profile anomalies, evidence for stratification, and effects of pulsation on spectral lines.
- Type
- Part 2.3. Chemically Peculiar Stars
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- Copyright © Astronomical Society of the Pacific 2002