Planetary migration in wind-fed non-stationary accretion disks in binary systems

Open Access

Table 1

Main free parameters of the binary used for modeling.

M₂ (M_⊙)	M_1,init (M_⊙)	M_1,final (M_⊙)	a_init (AU)	a_final (AU)
1.0	1.7	0.55	[10.0,100.0]	[17.1,173.5]
1.0	3.0	0.58	[10.0,100.0]	[24.1,248.7]
1.0	5.0	0.82	[10.0,100.0]	[30.4,320.2]
1.0	7.0	0.93	[10.0,100.0]	[36.5,387.5]

Notes. The columns show the secondary component mass M₂, the donor initial mass M_1,init, the donor final mass M_1,final, the binary initial major semi-axis range a_init, the binary final major semi-axis range a_final. Eccentricity of the system is assumed to be zero, e = 0.

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