Abstract
We analyze a high-resolution, high signal-to-noise spectrum of the carbon-rich, extremely metal-poor star CS29498-043, obtained with the Subaru Telescope High Dispersion Spectrograph. We find its iron abundance is extremely low ([Fe/H] = -3.7), placing it among the few stars known with [Fe/H]
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CITATION STYLE
APA
Aoki, W., Norris, J. E., Ryan, S. G., Beers, T. C., & Ando, H. (2002). Chemical Composition of the Carbon-rich, Extremely Metal Poor Star CS 29498−043: A New Class of Extremely Metal Poor Stars with Excesses of Magnesium and Silicon. The Astrophysical Journal, 576(2), L141–L144. https://doi.org/10.1086/343761
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