  We present the first time abundance analysis of a very metal-poor
carbon-enhanced star CD-27 14351 based on a high resolution (R ~ 48000) FEROS
spectrum. Our abundance analysis performed using Local Thermodynamic
Equilibrium (LTE) model atmospheres shows that the object is a cool star with
stellar atmospheric parameters, effective temperature Teff = 4335 K, surface
gravity log g = 0.5, microturbulence = 2.42 km/s, and, metallicity [Fe/H] =
-2.6. The star exhibits high carbon and nitrogen abundances with [C/Fe] = 2.89
and [N/Fe] = 1.89. Overabundances of neutron-capture elements are evident in
Ba, La, Ce, and Nd with estimated [X/Fe] > 1, the largest enhancement being
seen in Ce with [Ce/Fe] = 2.63. While the first peak s-process elements Sr and
Y are found to be enhanced with respect to Fe, ([Sr/Fe] = 1.73 and [Y/Fe] =
1.91) the third peak s-process element Pb could not be detected in our spectrum
at the given resolution. Europium, primarily a r-process element also shows an
enhancement with [Eu/Fe] = 1.65. With [Ba/Eu] = 0.12 the object CD-27 14351
satisfies the classification criterion for CEMP-r/s star. The elemental
abundance distributions observed in this star is discussed in light of chemical
abundances observed in other CEMP stars from literature.
