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2008

Type II Migration: Varying Planet Mass and Disc Viscosity

Edgar, Richard G.

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This paper continues an earlier study of giant planet migration, examining the effect of planet mass and disc viscosity on the migration rate.

We find that the migration rate of a gap-opening planet varies systematically with the planet's mass, as predicted in our earlier work.
However, the variation with disc viscosity appears to be much weaker than expected.

Type II Migration: Varying Planet Mass and Disc Viscosity · Around

Built on

MNRAS 277
Original
Syer, D. and Clarke, C. J.: 1995, · 1995
Earlier work this paper cites.

Similar

MNRAS 307
Ivanov, P. B., Papaloizou, J. C. B., and Polnarev, A. G.: 1999, · 1999
Cited alongside, same era.
A&AS 141
Masset, F.: 2000a,
Cited in the paper.
in ASP Conf. Ser. 219: Disks, Planetesimals, and Planets
Masset, F. S.: 2000b,
Cited in the paper.

Then

MNRAS 370
de Val-Borro, M., Edgar, R. G., Artymowicz, P., Ciecielag, P., Cresswell, P., D’Angelo, G., Delgado-Donate, E. J., Dirksen, G., Fromang, S., Gawryszczak, A., Klahr, H., Kley, W., Lyra, W., Masset, F., Mellema, G., Nelson, R. P., Paardekooper, S.-J., Peplinski, A., Pierens, A., Plewa, T., Rice, K., Schäfer, C., and Speith, R.: 2006, · 2006
Later among the works it cites.

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