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Nucleonic matter is described within a su(2) extended Nambu-Jona-Lasiniomodel. Several parametrizations with different nuclear matter saturationproperties are proposed. At subsaturation, nuclear pasta phases are calculatedwithin two methods: the coexistence-phases approximation and the compressibleliquid drop model, with the surface tension coefficient determined using ageometrical approach at zero temperature. An unified equation of state ofstellar matter for the inner crust, with the nuclear pasta phases, and the coreis calculated. The mass and radius of neutron stars within this framework areobtained for several families of hadronic and hybrid stars. The quark phase ofhybrid stars is described within the su(3) NJL model including a vector term.Stellar macroscopic properties are in accordance with some of the recentresults in the literature.

Neutron stars: from the inner crust to the core with the (Extended) Nambu-Jona-Lasinio model