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Table 1

The combinations of input parameters for the models of M-type AGB stars, sorted according to luminosity.

Model series M L T P(L) Δup log ngr/nH
[M] [L] [K] [d] [km s-1] [a, b, c, d]

L50 1 5000 2600–3000 310 3.0, 4.0 −16.0, −15.5, −15.0, −14.5
L70 1 7000 2600–3100 395 3.0, 4.0 −16.0, −15.5, −15.0, −14.5
L10 1 10 000 2600–3200 525 2.0, 3.0 −16.0, −15.5, −15.0, −14.5

Notes. The columns list stellar mass M, stellar luminosity L, effective temperature T of the star, pulsation period P, piston velocity amplitude Δup and the assumed seed particle abundance ngr/nH. The pulsation period is derived from the period-luminosity relation presented in Feast et al. (1989).

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