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Home All issues Volume 626 (June 2019) A&A, 626 (2019) A100 Full HTML
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Table 1

Fundamental parameters (stellar, pulsation, and dust parameters) covered in the grid of DARWIN models for M-type AGB stars.

M* log (L* ∕L⊙) T* P up fL log(nd∕nH)
(M⊙) (K) (d) (km s−1)
0.75 2.95 2200, 2300, …, 3000 101 2, 3, 4 2 − 14.5, − 15.0
3.10 2200, 2300, …, 3000 132 2, 3, 4 2 − 14.5, − 15.0
3.25 2200, 2300, …, 3000 171 2, 3, 4 2 − 14.5, − 15.0
3.40 2200, 2300, …, 3000 222 2, 3, 4 2 − 14.5, − 15.0
3.55 2200, 2300, …, 3200 288 2, 3, 4 2 − 14.5, − 15.0
3.70 2200, 2300, …, 3200 373 2, 3, 4 2 − 14.5, − 15.0
3.85 2200, 2300, …, 3300 485 2, 3, 4 2 − 14.5, − 15.0
1.0 3.10 2200, 2300, …, 3000 132 2, 3, 4 2 − 14.5, − 15.0
3.25 2200, 2300, …, 3000 171 2, 3, 4 2 − 14.5, − 15.0
3.40 2200, 2300, …, 3000 222 2, 3, 4 2 − 14.5, − 15.0
3.55 2200, 2300, …, 3000 288 2, 3, 4 2 − 14.5, − 15.0
3.70 2200, 2300, …, 3000 373 2, 3, 4 2 − 14.5, − 15.0
3.85 2200, 2300, …, 3200 485 2, 3, 4 2 − 14.5, − 15.0
4.00 2200, 2300, …, 3200 629 2, 3, 4 2 − 14.5, − 15.0
4.15 2200, 2300, …, 3200 817 2, 3, 4 2 − 14.5, − 15.0
1.5 3.25 2200, 2300, …, 3000 171 2, 3, 4 2 − 14.5, − 15.0
3.40 2200, 2300, …, 3000 222 2, 3, 4 2 − 14.5, − 15.0
3.55 2200, 2300, …, 3000 288 2, 3, 4 2 − 14.5, − 15.0
3.70 2200, 2300, …, 3000 373 2, 3, 4 2 − 14.5, − 15.0
3.85 2200, 2300, …, 3200 485 2, 3, 4 2 − 14.5, − 15.0
4.00 2200, 2300, …, 3200 629 2, 3, 4 2 − 14.5, − 15.0
4.15 2200, 2300, …, 3200 817 2, 3, 4 2 − 14.5, − 15.0
4.30 2200, 2300, …, 3200 1060 2, 3, 4 2 − 14.5, − 15.0
2.0 3.55 2200, 2300, …, 3000 288 2, 3, 4 2 − 14.5, − 15.0
3.70 2200, 2300, …, 3000 373 2, 3, 4 2 − 14.5, − 15.0
3.85 2200, 2300, …, 3200 485 2, 3, 4 2 − 14.5, − 15.0
4.00 2200, 2300, …, 3100 629 2, 3, 4 2 − 14.5, − 15.0
4.15 2200, 2300, …, 3200 817 2, 3, 4 2 − 14.5, − 15.0
4.30 2200, 2300, …, 3200 1060 2, 3, 4 2 − 14.5, − 15.0
4.45 2200, 2300, …, 3200 1376 2, 3, 4 2 − 14.5, − 15.0
4.60 2200, 2300, …, 3300 1786 2, 3, 4 2 − 14.5, − 15.0
2.5 3.70 2200, 2300, …, 3000 373 2, 3, 4 2 − 14.5, − 15.0
3.85 2200, 2300, …, 3000 485 2, 3, 4 2 − 14.5, − 15.0
4.00 2200, 2300, …, 3200 629 2, 3, 4 2 − 14.5, − 15.0
4.15 2200, 2300, …, 3200 817 2, 3, 4 2 − 14.5, − 15.0
4.30 2200, 2300, …, 3200 1060 2, 3, 4 2 − 14.5, − 15.0
4.45 2200, 2300, …, 3200 1376 2, 3, 4 2 − 14.5, − 15.0
4.60 2200, 2300, …, 3300 1786 2, 3, 4 2 − 14.5, − 15.0
3.0 3.85 2200, 2300, …, 3000 485 2, 3, 4 2 − 14.5, − 15.0
4.00 2200, 2300, …, 3100 629 2, 3, 4 2 − 14.5, − 15.0
4.15 2200, 2300, …, 3200 817 2, 3, 4 2 − 14.5, − 15.0
4.30 2200, 2300, …, 3200 1060 2, 3, 4 2 − 14.5, − 15.0
4.45 2200, 2300, …, 3200 1376 2, 3, 4 2 − 14.5, − 15.0
4.60 2200, 2300, …, 3200 1786 2, 3, 4 2 − 14.5, − 15.0

Notes. The columns show stellar mass M*, stellar luminosity L*, effective temperature T*, pulsation period P, piston velocity up, the scaling factor for the luminosity amplitude fL, and the seed particle abundance nd∕nH. The pulsation period is not an independent parameter, but is set according to the period-luminosity relation by Whitelock et al. (2009).

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