  We consider a TeV scale resonant lepogenesis within type-I seesaw mechanism.
We show that a concrete model based on $A_4$ flavor symmetry with a scaling
ansatz in the neutrino Dirac mass matrix and a retro-circulant heavy Majorana
mass matrix can be realized. The full Yukawa coupling matrix $Y_{\nu}$ can be
fully reconstructed from the low energy neutrino oscillations data and the
quasi-degenerate heavy Majorara neutrino masses. We have carried out a detailed
numerical analysis to constrain the Dirac neutrino mass matrix elements. In
particular, it was found that its diagonal elements lie near or below the MeV
region. Furthermore, we have investigated the allowed regions in the parameter
space of the model consistent with both low energy neutrino oscillations data
and resonant leptogenesis leading to the observed baryon asymmetry of the
universe. Finally, the model has an imperative prediction on the allowed space
for the effective Majorana neutrino mass $|m_{ee}|$ in order to account for the
observed baryon asymmetry.
