Impact of H I cooling and study of accretion disks in asymptotic giant branch wind-companion smoothed particle hydrodynamic simulations

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Table 5

Disk properties v05e50 at different orbital phases.

t (yr)	ϕ	r_disk (au)	M_disk (M_⊙)	H_max (au)	${\tilde{H}}_{max}$ $\[\tilde{H}_{\max }\]$ (au)
85.5	0.16 π	0.70	2.10 × 10⁻⁷	0.13	0.30
88.3	1.02 π	0.71	2.07 × 10⁻⁷	0.18	0.34
90.6	1.77 π	0.69	1.69 × 10⁻⁷	0.13	0.31
93.0	2.00 π	0.77	1.65 × 10⁻⁷	0.16	0.38

Notes. Disk radius r_disk, mass M_disk, and scale heights H_max and ${\tilde{H}}_{max}$ $\[\tilde{H}_{\max }\]$ as calculated from the analysis described in Sect. 4.4, at four consecutive orbital phases ϕ for model v05e50 (corresponding to the plots in Fig. 16).

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