On the Limits of Seismic Inversions for Radial Differential Rotation of Solar-Type Stars

Seismic data contains information on stellar internal rotation, which plays an important role on dynamo models. Due to the uncertainties on the observations and stellar models, determining internal rotation of main-sequence solar-type stars has been challenging. Here, we use artificial rotational splittings for two-zone profiles to explore the limitations to constrain internal rotation profiles.