* Astronomy

Title: Carbon and Strontium Abundances of Metal-Poor Stars
Authors: David K. Lai (UCSC), Jennifer A. Johnson (OSU), Michael Bolte (UCSC), Sara Lucatello (INAF-OAPD)

We present carbon and strontium abundances for 100 metal-poor stars measured from R ~ 7000 spectra obtained with the Echellette Spectrograph and Imager at the Keck Observatory. Using spectral synthesis of the G-band region, we have derived carbon abundances for stars ranging from [Fe/H]=-1.3 to [Fe/H]=-3.8. The formal errors are ~ 0.2 dex in [C/Fe]. The strontium abundance in these stars was measured using spectral synthesis of the resonance line at 4215 {\AA}. Using these two abundance measurements along with the barium abundances from our previous study of these stars, we show it is possible to identify neutron-capture-rich stars with our spectra. We find, as in other studies, a large scatter in [C/Fe] below [Fe/H] = -2. Of the stars with [Fe/H]<-2, 9 ± 4% can be classified as carbon-rich metal-poor stars. The Sr and Ba abundances show that three of the carbon-rich stars are neutron-capture-rich, while two have normal Ba and Sr. This fraction of carbon enhanced stars is consistent with other studies that include this metallicity range.

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