Extremely Metal-poor Stars. IX. CS 22949-037 and the Role of Hypernovae
We have obtained high-resolution spectra of the extremely metal-poor star CS 22949-037 ([Fe/H] = -3.79) in the region of the ultraviolet NH bands at 3360-3370 Å, which confirm our earlier report that it exhibits extreme nitrogen enhancement. We find [N/F
|Collections||ANU Research Publications|
|Source:||Astrophysical Journal, The|
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