Nova Movies

Fig. 1: Evolution of a CO nova with M_wd=1.2M_sun, T_wd=30MK, and mass accretion rate dM/dt=1e-10 M_sun/yr.

Fig. 4: Relative changes of abundances (with respect to the solar ones) in nuclear reactions occuring near the base of the envelope during the first cycle (models 4340 to 4670) of the nova evolution shown in Fig 1.

Fig. 5: Changes of abundances in nuclear reactions occurring near the base of the accreted envelope during the first cycle (models 4340 to 4670) of the nova evolution shown in Fig 1.