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Modelling NIR molecular lines for Miras

W. Nowotny·S. Hoefner·T. Lebzelter·B. Aringer·J. Hron
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Abstract

The atmospheric structure of Mira variables is considerably influenced by pulsation. Molecular absorption lines in the near-infrared (NIR), especially second overtone CO lines, show therefore a characteristic behaviour in time-series of high-resolution spectra. We computed synthetic CO line profiles based on a new dynamic model atmosphere and derived radial velocities (RVs) from the Doppler shifted lines. For the first time, we could quantitatively reproduce observations of the very typical, discontinuous RV curves.

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W. Nowotny, S. Hoefner, T. Lebzelter, B. Aringer, J. Hron. 2005-07-21. Modelling NIR molecular lines for Miras. https://arxiv.org/abs/astro-ph/0507476

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