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Cited article:

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The origin of planetary system architectures - I. Multiple planet traps in gaseous discs

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A torque formula for non-isothermal Type I planetary migration - II. Effects of diffusion

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A torque formula for non-isothermal type I planetary migration - I. Unsaturated horseshoe drag

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Planet migration: self-gravitating radiation hydrodynamical models of protoplanets with surfaces

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The Astrophysical Journal 715 (2) L68 (2010)
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Application of recent results on the orbital migration of low mass planets: convergence zones

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Proceedings of the International Astronomical Union 6 (S276) 72 (2010)
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MIGRATION OF A MOONLET IN A RING OF SOLID PARTICLES: THEORY AND APPLICATION TO SATURN'S PROPELLERS

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SATURATED TORQUE FORMULA FOR PLANETARY MIGRATION IN VISCOUS DISKS WITH THERMAL DIFFUSION: RECIPE FOR PROTOPLANET POPULATION SYNTHESIS

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PLANETESIMAL AND PROTOPLANET DYNAMICS IN A TURBULENT PROTOPLANETARY DISK: IDEAL UNSTRATIFIED DISKS

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The Astrophysical Journal 707 (2) 1233 (2009)
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On corotation torques, horseshoe drag and the possibility of sustained stalled or outward protoplanetary migration

S.-J. Paardekooper and J. C. B. Papaloizou
Monthly Notices of the Royal Astronomical Society 394 (4) 2283 (2009)
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