Magnetically driven winds from accretion disks in post-asymptotic giant branch binaries

Open Access

Fig. 10.

Mass accretion rate effect. These dynamic spectra all have the same input parameters (Tables 1 and 2) except for the mass accretion rate. These rates are, from top to bottom: 10⁻³ M_⊙ yr⁻¹, 10⁻⁴ M_⊙ yr⁻¹, and 10⁻⁵ M_⊙ yr⁻¹.

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