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).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.