Open Access

Fig. A.1

image

Scheme of the dependences in the code. We first initialize the values of a, Lc, and Lr. At eachtime step, the torques are computed from the current state of the system, the stellar evolution variables, and the results of starAML. Subsequently, the time derivatives ȧ, , and are computed from the torques. This iterative integration goes on until the age of the system is greater than the limit age we set for the computation.

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