We discuss how the cosmological baryon asymmetry can be achieved by the lepton family asymmetries of heavy Majorana neutrino decays and how the lepton family asymmetries are related to $CP$ violation in neutrino oscillation, in the minimal seesaw model with two heavy Majorana neutrinos. We derive the most general formula for $CP$ violation in neutrino oscillation in terms of the heavy Majorana masses and Yukawa mass term. It is shown that the formula is very useful to classify several models in which $e$, $\ensuremath{\mu}$, and $\ensuremath{\tau}$ leptogenesis can be separately realized and to see how they are connected with low energy $CP$ violation. To make the models predictive, we take texture with two zeros in the Dirac matrix. In particular, we find some interesting cases in which $CP$ violation in neutrino oscillation can happen while lepton family asymmetries do not exist at all. On the contrary, we can find $e$-, $\ensuremath{\mu}$-, and $\ensuremath{\tau}$-leptogenesis scenarios in which the cosmological $CP$ violation and low energy $CP$ violation measurable via neutrino oscillations are very closely related to each other. By determining the allowed ranges of the parameters in the models, we predict the sizes of $CP$ violation in neutrino oscillation and $|{V}_{e3}^{\mathrm{MNS}}|$. Finally, the leptonic unitarity triangles are reconstructed.