par Escorza Santos, Ana
;Boffin, Henri
;Jorissen, Alain
;Van Eck, Sophie
;Siess, Lionel
;Van Winckel, Hans;Karinkuzhi, Drisya
;Shetye, Shreeya
;Pourbaix, Dimitri 
Référence Astronomy & astrophysics, 608, A100
Publication Publié, 2017-12
;Boffin, Henri
;Jorissen, Alain
;Van Eck, Sophie
;Siess, Lionel
;Van Winckel, Hans;Karinkuzhi, Drisya
;Shetye, Shreeya
;Pourbaix, Dimitri 
Référence Astronomy & astrophysics, 608, A100
Publication Publié, 2017-12
Article révisé par les pairs
| Résumé : | We noticed that the values of P and to a lower extent P shown in Fig. 17 of our article Escorza et al. (2017) had been wrongly estimated because the algorithm to find the maximum stellar radius contained an error. In the original plot, we did not discard the core-He burning phase and for stars (Figure Presented). |



