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In the present work,we used five different versions of the quark-meson coupling(QMC)model to com-pute astrophysical quantities related to the GW170817 event and the neutron star cooling process.Two of the mod-els are based on the original bag potential structure and three versions consider a harmonic oscillator potential to confine quarks.The bag-like models also incorporate the pasta phase used to describe the inner crust of neutron stars.With a simple method studied in the present work,we show that the pasta phase does not play a significant role.Moreover,the QMC model that satisfies the GW 170817 constraints with the lowest slope of the symmetry en-ergy exhibits a cooling profile compatible with observational data.