Apsidal motion in massive eccentric binaries: the case of cpd-41° 7742, and hd 152218 revisited

HIGHLIGHTS

• who: Rosu S. et al. from the Stellar structure and evolution models We computed stellar evolution models with the Code Liu00e9geois d`u00c9volution Stellaire, (Clu00e9s, Scuflaire et_al, see also Rosu et_al , for an overview of the main features of Clu00e9s and its minimisation routine min-Clu00e9s used in the present context). The aim of the present analysis is to see whether standard models reproducing the stellar physical properties are also capable of reproducing the apsidal motion rate inferred in Sect., . For all models built, we adopted the mass-loss rate scaling factor u03be=1. In a first . . .
  

   

  

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