Corotation torques in the solar nebula - The cutoff function

Details Corotation torques in the solar nebula - The cutoff function Corotation torques in the solar nebula - The cutoff function

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...336..526w&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 336, Jan. 1, 1989, p. 526-538.

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24

Corotation, Density Wave Model, Planetary Evolution, Solar Corona, Solar System, Computational Astrophysics, Orbital Mechanics, Perturbation Theory

Scientific paper

The behavior of high-order corotation resonances in a disk of finite thickness is examined. The torque exerted at an mth-order resonance is determined by employing a vertically averaged disturbing function, and the ratio of this torque to that exerted on a cold, two-dimensional disk is identified as the so-called torque cutoff function. This function is then used to calculate contributions from the corotation torques to eccentricity variations of a perturber's orbit assumed orbiting in the disk.

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