How to disentangle geometry and mass-loss rate from AGB-star spectral energy distributions -- The case of EP Aqr

J. Wiegert, M. A. T. Groenewegen, A. Jorissen +2

High-angular-resolution observations of asymptotic giant branch (AGB) stars often reveal non-spherical morphologies for the gas and dust envelopes. We aim to make a pilot study to…