3D simulations of M star atmosphere velocities and their influence on molecular FeH lines

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Volume 508 / No 3 (December IV 2009)

A&A, 508 3 (2009) 1429-1442

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Table 1:

Overview of different model quantities for models at constant $T_{{\rm eff}}$ and different $\log{g}$ (upper part) and at constant $\log{g}$ and different $T_{{\rm eff}}$ (lower part).
Model code	Size(x, y, z) [km]	Grid points (nx, ny, nz)	$H_{\rm p}$ [km]^a	z-size [ $H_{\rm p}$ ]	$T_{{\rm eff}}$ [K]	$\log{g}$ [cgs]
d3t33g30mm00w1	85 000 $\times$ 85 000 $\times$ 58 350	180 $\times$ 180 $\times$ 150	2821	20.7	3240	3.0
d3t33g35mm00w1	28 000 $\times$ 28000 $\times$ 11 500	180 $\times$ 180 $\times$ 150	826	13.9	3270	3.5
d3t33g40mm00w1	7750 $\times$ 7750 $\times$ 1850	150 $\times$ 150 $\times$ 150	250	7.4	3315	4.0
d3t33g50mm00w1	300 $\times$ 300 $\times$ 260	180 $\times$ 180 $\times$ 150	18	14.5	3275	5.0
d3t40g45mm00n01	4700 $\times$ 4700 $\times$ 1150	140 $\times$ 140 $\times$ 141	109	10.6	4000	4.5
d3t38g49mm00w1	1900 $\times$ 1900 $\times$ 420	140 $\times$ 140 $\times$ 150	36	11.7	3820	4.9
d3t35g50mm00w1	1070 $\times$ 1070 $\times$ 290	180 $\times$ 180 $\times$ 150	20	14.5	3380	5.0
d3t28g50mm00w1	370 $\times$ 370 $\times$ 270	250 $\times$ 250 $\times$ 140	13	20.8	2800	5.0
d3t25g50mm00w1	240 $\times$ 240 $\times$ 170	250 $\times$ 250 $\times$ 120	12	14.2	2575	5.0

^a At $\tau=1$ .

Source LaTeX | All tables | In the text

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