On the tidal interaction between protoplanets and the protoplanetary disk. III - Orbital migration of protoplanets Export

@article{citeulike:3651930, abstract = {The tidal interaction between a protoplanet and a gaseous protoplanetary disk is investigated, and the dynamical evolution of the disk and the orbital migration of the protoplanet in a self-consistent manner is considered. It is shown that the orbital migration of a protoplanet does not suppress the tendency for tidal truncation in the vicinity of its orbit. If the necessary condition for tidal truncation is satisfied, the protoplanet induces a tidal feedback mechanism that regulates the rate of angular momentum transfer between the protoplanet and the disk. Significant orbital migration can only occur on the viscous evolution time scale of the disk.}, author = {Lin, D. N. C. and Papaloizou, J.}, citeulike-article-id = {3651930}, citeulike-linkout-0 = {http://dx.doi.org/10.1086/164653}, citeulike-linkout-1 = {http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=1986ApJ...309..846L}, doi = {10.1086/164653}, journal = {Astrophys. J.}, keywords = {angular, evolution, feedback, models, momentum, orbit, perturbation, planetary, protoplanets, stellar, tides, transfer}, month = {October}, pages = {846--857}, posted-at = {2008-11-21 15:59:30}, priority = {4}, title = {On the tidal interaction between protoplanets and the protoplanetary disk. III - Orbital migration of protoplanets}, url = {http://dx.doi.org/10.1086/164653}, volume = {309}, year = {1986} }

TY - JOUR ID - citeulike:3651930 L3 - citeulike-article-id:3651930 N2 - The tidal interaction between a protoplanet and a gaseous protoplanetary disk is investigated, and the dynamical evolution of the disk and the orbital migration of the protoplanet in a self-consistent manner is considered. It is shown that the orbital migration of a protoplanet does not suppress the tendency for tidal truncation in the vicinity of its orbit. If the necessary condition for tidal truncation is satisfied, the protoplanet induces a tidal feedback mechanism that regulates the rate of angular momentum transfer between the protoplanet and the disk. Significant orbital migration can only occur on the viscous evolution time scale of the disk. JF - Astrophys. J. EP - 857 TI - On the tidal interaction between protoplanets and the protoplanetary disk. III - Orbital migration of protoplanets VL - 309 SP - 846 KW - angular KW - evolution KW - feedback KW - models KW - momentum KW - orbit KW - perturbation KW - planetary KW - protoplanets KW - stellar KW - tides KW - transfer AU - Lin, DNC AU - Papaloizou, J PY - 1986/October// UR - http://dx.doi.org/10.1086/164653 ER -