Figure 4From: Orbital evolution of planetesimals in gaseous disks C 1(i)≡(Δ e) e=1 τ 0(q)/T K(q) and \(C_{2}(i) \equiv (\langle \dot i \rangle /i \langle \dot e \rangle)_{e =1}\) derived from the combined equations (Equations 14 to 16).Back to article page