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
Author supplied keywords
Cite
CITATION STYLE
APA
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
Register to see more suggestions
Mendeley helps you to discover research relevant for your work.
Already have an account? Sign in
Sign up for free