A high-resolution spectral analysis of three carbon-enhanced metal-poor stars
We present results of an analysis of high-resolution spectra (R ∼ 50000), obtained with the Subaru Telescope High Dispersion Spectrograph, of two carbon-enhanced metal-poor (CEMP) stars selected from the Hamburg/European Southern Observatory prism surve
|Collections||ANU Research Publications|
|Source:||Monthly Notices of the Royal Astronomical Society|
|01_Goswami_A_high-resolution_spectral_2006.pdf||721.08 kB||Adobe PDF||Request a copy|
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