Three-dimensional Interaction between a Planet and an Isothermal Gaseous
Disk. III. Locally Isothermal Cases
Three-dimensional Interaction between a Planet and an Isothermal Gaseous
Disk. III. Locally Isothermal Cases
We performed linear calculations to determine the Type I planetary migration rate for three-dimensional locally isothermal disks with radial temperature gradients. For 3D disks with radial temperature gradients, the linear wave equation has a divergent term of the third pole, which makes corotation a non-removal singularity. We suppressed the divergence …