The IACOB project - IV. New predictions for high-degree non-radial mode instability domains in massive stars and their connection with macroturbulent broadening

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Table 1

Global stellar parameters of 11 selected models: mass, effective temperature, gravity, the quantity L defined as , central hydrogen abundance, and dynamical time in hour.

	M/M_⊙	log T_eff	log g	log L/ L_⊙	X_c	τ_dyn

A	50	4.60	3.79	3.99	0.363	20.8
B	50	4.50	3.33	4.06	0.161	44.3
C	30	4.38	2.97	3.95	0.000	76.3
D	15	4.42	3.69	3.38	0.140	19.9
E	15	4.36	3.36	3.49	0.000	34.8
F	15	4.22	2.79	3.49	0.000	93.9
G	6	4.30	4.32	2.26	0.697	5.34
H	6	4.25	3.96	2.43	0.303	9.88
I	6	4.20	3.67	2.51	0.035	16.5
J	8	4.33	3.97	2.72	0.331	10.5
K	4	4.14	4.00	1.96	0.316	8.45

Notes. The location of these models in the spectroscopic HR diagram can be seen in Figs. 2 and 3.

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