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On reconstruit la courbe de lumiere bolometrique d'une supernova de type Ia a partir de la photometrie UBVRI et des spectres integres. On la compare a une courbe de lumiere calculee a partir d'un modele. On ne trouve aucun ajustement satisfaisant avec les donnees car la luminosite theorique diminue trop lentement

The bolometric light curve of a carbon deflagration supernova