Spiral density waves and vertical circulation in protoplanetary discs

Spiral density waves dominate several facets of accretion disc dynamics – planet-disc interactions and gravitational instability (GI) most prominently. Though they have been examined thoroughly in two-dimensional simulations, their vertical structures in the non-linear regime are somewhat unexplored...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2018-06, Vol.476 (4), p.5115-5126
Hauptverfasser:	Riols, A, Latter, H
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrophysics Physics
Online-Zugang:	Volltext
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