Estimates for carbon-enhanced metal-poor stars from near-infrared spectroscopy

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Abstract

We report on oxygen abundances determined from medium-resolution near-infrared spectroscopy for a sample of 57 carbon-enhanced metal-poor (CEMP) stars selected from the Hamburg/ESO Survey. The majority of our program stars exhibit oxygen-to-iron ratios in the range +0.5

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Kennedy, C. R., Sivarani, T., Beers, T. C., Lee, Y. S., Placco, V. M., Rossi, S., … Plez, B. (2011). Estimates for carbon-enhanced metal-poor stars from near-infrared spectroscopy. Astronomical Journal, 141(3). https://doi.org/10.1088/0004-6256/141/3/102

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