  We present elemental abundance results from high resolution spectral analysis
of three nitrogen-enhanced barium stars. The analysis is based on spectra
obtained with the FEROS attached to 1.52m telescope at ESO, Chile. The spectral
resolution is R~48000 and the spectral coverage spans from 3500-9000\AA\,. For
the objects HD 51959 and HD 88035, we present the first time abundance analyses
results. Although a few studies are available in literature on the object HD
121447, the results are significantly different from each other. We have
therefore carried out a detailed chemical composition study for this object
based on a high resolution spectrum with high S/N ratio, for a better
understanding of the origin of the abundance patterns observed in this star.
Stellar atmospheric parameters, the effective temperature, surface gravity,
microturbulence and metallicity of the stars are determined from the LTE
analysis using model atmospheres. The metallicity of HD 51959 and HD 88035 are
found to be near-solar; they exhibit enhanced abundances of neutron-capture
elements. HD 121447 is found to be moderately metal-poor with [Fe/H]=-0.65.
While carbon is near-solar in the other two objects, HD 121447 shows carbon
enhancement at a level, [C/Fe]=0.82. Neutron-capture elements are highly
enhanced with [X/Fe]>2 (X: Ba, La, Pr, Nd, Sm) in this object. The alpha- and
iron-peak elements show abundances very similar to field giants with the same
metallicity. From kinematic analysis all the three objects are found to be
members of thin disk population with a high probability of 0.99, 0.99 and 0.92
for HD 51959, HD 88035 and HD 121447 respectively.
