167 citations · 817 across the 17 of their papers we have counts for
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AGB nucleosynthesis at low metallicity: what can we learn from carbon- and s-elements-enhanced metal-poor stars
Carlo Abate, Onno R. Pols, Robert G. Izzard +1
CEMP-s stars are very metal-poor stars with enhanced abundances of carbon and s-process elements. They form a significant proportion of the very metal-poor stars in the Galactic ha…
The elusive origin of Carbon-Enhanced Metal-Poor stars
C. Abate, O. R. Pols, R. G. Izzard +2
Carbon-enhanced metal-poor (CEMP) stars count for 9-25% of all the very metal-poor stars of the halo. In at least some CEMP stars the chemical enrichment is believed to be due to w…
Wind Roche-lobe overflow: Application to carbon-enhanced metal-poor stars
C. Abate, O. R. Pols, R. G. Izzard +2
Carbon-enhanced metal-poor stars (CEMP) are observed as a substantial fraction of the very metal-poor stars in the Galactic halo. Most CEMP stars are also enriched in s-process ele…