Measurements of the $^3$He and $D$ components in cosmic rays with the AMS-02 experiment

The $^3$He/$^4$He and $D/p$ flux ratios in cosmic rays (CR) are two of the most valuable tools for understanding the propagation of CR in the galaxy and constrain the models that describe it. In this work, two new preliminary measurements of $^3$He/$^4$He and $D/p$ flux ratios are presented, each obtained from the data of the AMS-02 experiment.