Flattened broad-emission-line geometries (Keplerian disk or equatorial wind) are favored over a polar wind by Hα microlensing in HE0435-1223, with a slight preference for the Keplerian disk under an independent continuum-size constraint.
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Constraining the geometry and kinematics of the quasar broad emission line region using gravitational microlensing. II. Comparing models with observations in the lensed quasar HE0435-1223
Flattened broad-emission-line geometries (Keplerian disk or equatorial wind) are favored over a polar wind by Hα microlensing in HE0435-1223, with a slight preference for the Keplerian disk under an independent continuum-size constraint.