Asteroseismic study of helium and heavy element diffusion in solar-type stars

Free Access

Issue		A&A Volume 508, Number 2, December III 2009


Page(s)		849 - 854
Section		Stellar structure and evolution
DOI		https://doi.org/10.1051/0004-6361/200912417
Published online		21 October 2009

Online Material

Table 1: The average large and small separations $\langle \Delta\nu_{0} \rangle$ , $\langle d_{02} \rangle$ , $\langle d_{13} \rangle$ for models with Z_i = 0.03.

Table 2: The average large and small separations $\langle \Delta\nu_{0} \rangle$ , $\langle d_{02} \rangle$ , $\langle d_{13} \rangle$ for models with Z_i = 0.025.

Table 3: The average large and small separations $\langle \Delta\nu_{0} \rangle$ , $\langle d_{02} \rangle$ , $\langle d_{13} \rangle$ for models with Z_i = 0.02.

Table 4: The average large and small separations $\langle \Delta\nu_{0} \rangle$ , $\langle d_{02} \rangle$ , $\langle d_{13} \rangle$ for models with Z_i = 0.015.

Table 5: The average large and small separations $\langle \Delta\nu_{0} \rangle$ , $\langle d_{02} \rangle$ , $\langle d_{13} \rangle$ for models with Z_i = 0.01.

Table 6: The average large and small separations $\langle \Delta\nu_{0} \rangle$ , $\langle d_{02} \rangle$ , $\langle d_{13} \rangle$ for models with Z_i = 0.005.

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