Merging in the common envelope and the origin of early R-type stars

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Table 5

Selected properties for the three models listed in Table 1, computed by assuming rigid body rotation in the He core.

	M1	M2	M3

M _c1 ^a	0.2036	0.1967	0.2307
M _c2 ^a	0.3536	0.3967	0.4307
M _c3 ^a	0.4067	0.4103	0.4308
M _fl ^a	0.0000	0.0375	0.0000
ΔM_fl^a	0.3870	0.3550	0.2690

Notes.

In M_⊙ unit.

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