Structure and evolution of a tidally heated star | Astronomy & Astrophysics (A&A)

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Table 6.

Ages and events in MESA models.

Age	Event
(Gyr)
	Standard model h0:
9.207	Core H-abundance [N(H)] ≃ 0.0001
10.758	R₁ ≃ 1.5 R_⊙
11.644	End of calculation; R₁ = 2.25 R_⊙
	Set 2:
9.247	N(H) ≃ 0.0001, model h1
9.381	N(H) ≃ 0.0001, model h10
	Set 3:
9.237	N(H) ≃ 0.0001, model h1
9.3591	N(H) ≃ 0.0001, model h10
10.708	R₁ ≃ 1.5 R_⊙, model h1
9.765	R₁ ≃ 1.5 R_⊙, model h10
11.673	R₁ = 2.25 R_⊙ end of the run h1
11.728	R₁ = 2.25 R_⊙ end of the run h10

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