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A weakly non-linear theory for spiral density waves excited by accretion disc turbulence Weakly non-linear spiral density waves (2012)

First Author: Heinemann T

Attributed to: Accretion discs, Astrophysical dynamos, Planetary formation, Exoplanet systems, Solar and stellar phenomena and non equilibrium physical processes funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1111/j.1365-2966.2011.19763.x

Publication URI: http://dx.doi.org/10.1111/j.1365-2966.2011.19763.x

Type: Journal Article/Review

Parent Publication: Monthly Notices of the Royal Astronomical Society

Issue: 2