Extremely Metal-poor Stars. VII. The Most Metal-poor Dwarf, CS 22876-032
We report high-resolution, high signal-to-noise observations of the extremely metal-poor double-lined spectroscopic binary CS 22876-032. The system has a long period: P = 424.7 ± 0.6 days. It comprises two main-sequence stars having effective temperature
|Collections||ANU Research Publications|
|Source:||Astrophysical Journal, The|
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