Impact of helium diffusion and helium-flash-induced carbon production on gravity-mode pulsations in subdwarf B stars

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Table 1:

Blue edge in terms of $\log T_{\rm eff}$ of the g-mode instability strip for our sdB models^a.
Fe	Ni	H/He-	opacity	l
		diffusion		1	2	3	4
yes	yes	yes	OPAL	4.34	4.38	4.41	4.43
yes	yes	yes	OP	4.41	4.45	4.47	4.48
yes	yes	no	OP	4.38	4.43	4.45	4.47
yes	no	yes	OP	4.35	4.39	4.42	4.44

^aThe results for the first three assumptions are also shown in Fig. 6.

Source LaTeX | All tables | In the text

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