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

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

2004-07-16

arxiv.org/abs/astro-ph/0407340v1

Astronomy and Astrophysics

Astrophysics

To appear in the proceedings of the ESO Workshop on High Resolution Infrared Spectroscopy in Astronomy held in Garching, Germa

Scientific paper

10.1007/10995082_55

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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