Adding viscous shear heating to Ae disk models makes Hα emission much easier to produce for spectral types A2 and cooler, and this dependence is proposed as a new way to measure the disk viscosity parameter α, though the current data give inconsistent values.
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Using the Coolest Ae Stars to Constrain Circumstellar Disk Viscosity
Adding viscous shear heating to Ae disk models makes Hα emission much easier to produce for spectral types A2 and cooler, and this dependence is proposed as a new way to measure the disk viscosity parameter α, though the current data give inconsistent values.