The Abundance of Elements in Cool Stars, as Determined from High-Resolution, 1-5 Micron Spectroscopy

N. Ryde; B. Gustafsson; K. Eriksson; R. Wahlin

doi:10.1007/10995082_55

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arXiv · astro-ph/0407340

The Abundance of Elements in Cool Stars, as Determined from High-Resolution, 1-5 Micron Spectroscopy

N. Ryde·B. Gustafsson·K. Eriksson·R. Wahlin

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Abstract

We review the field of abundance determinations of elements in cool stars, with special interest paid to determinations based on analyses of high-resolution, 1-5 micron spectra. We discuss the current status, problems, and challenges of exploring high-resolution, near-infrared spectra. In particular, advantages and drawbacks are pointed out. A few examples of current, chemical-abundance determinations are high-lighted and, finally, we discuss the development

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N. Ryde, B. Gustafsson, K. Eriksson, R. Wahlin. 2004-07-16. The Abundance of Elements in Cool Stars, as Determined from High-Resolution, 1-5 Micron Spectroscopy. https://doi.org/10.1007/10995082_55

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