Pure-hydrogen 3D model atmospheres of cool white dwarfs

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Volume 552 (April 2013)

A&A, 552 (2013) A13

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Table 2

3D model atmospheres.

T_eff	log g	x × y × z	ln(P_bot/P_phot)^a	Time^b	3D log g corr.
(K)		(km) × (km) × (km)		(s)

5997	8.0	1.19 × 1.19 × 0.34	5.0	100	0.00
7012	8.0	1.19 × 1.19 × 0.38	4.2	60	–0.07
8032	8.0	1.40 × 1.40 × 0.43	3.7	60	–0.16
9035	8.0	1.58 × 1.58 × 0.51	3.3	10	–0.26
9520	8.0	2.06 × 2.06 × 0.62	3.8	10	–0.25
10 018	8.0	2.10 × 2.10 × 0.76	4.3	10	–0.24
10 530	8.0	2.24 × 2.24 × 0.88	3.6	10	–0.22
11 004	8.0	2.68 × 2.68 × 1.19	4.0	10	–0.15
11 531	8.0	3.65 × 3.65 × 1.69	3.6	10	–0.11
12 022	8.0	7.45 × 7.45 × 4.06	2.0	10	–0.07
12 505	8.0	7.45 × 7.45 × 4.08	1.9	10	–0.09
12 999	8.0	7.45 × 7.45 × 4.41	1.8	10	–0.09

Notes.

^(a)

P_bot is the pressure at the bottom layer and P_phot the pressure at τ_R = 2/3;

^(b)

total stellar time. For the three cooler models, the total time includes the initial 2D run as described in Sect. 3.3.

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