  Abundance analyses of the two newly discovered R Coronae Borealis (RCB) stars
ASAS-RCB-8 and ASAS-RCB-10 were conducted using high-resolution optical spectra
and model atmospheres. Their chemical compositions place the pair among the
majority class of RCBs. ASAS-RCB-10 is one of the most N-poor majority RCBs
with an above average O abundance. Relative to ASAS-RCB-10, ASAS-RCB-8 is H
poor by 1.6 dex, O-poor by 0.7 dex but N-rich by 0.8 dex suggesting a higher
contamination by CNO-cycled material.
