These instabilities are a key
mechanism for eliciting the transport
of angular momentum through nascent
planetary systems, and are very important to an overall understanding
of planet
formation.
Lloyd, J.P., Lunine, J.I., Mamajek, E., Spiegel, D.S., Covey, K.R., Shkolnik, E.L., Walkowicz, L., Chavez, M., Bertone, E., & Olmedo Aguilar, J.M., Targeting Young Stars with Kepler: Planet
Formation, Migration
Mechanisms and the Early History
of Planetary Systems, eprint arXiv: 1309 - 1520, 2013
Abstract: In recent years there have been many attempts to characterize the occurrence
of stellar, BD and
planetary - mass companions to solar - type stars, with the aim
of constraining
formation mechanisms.