Nonlocal density wave theory for gravitational instability of protoplanetary disks without sharp boundaries

DOI<link itemprop=identifier href="https://doi.org/10.1002/1521-3994(200008)321:3<181::AID-ASNA181>3.0.CO;2-6" /><181::AID-ASNA181>3.0.CO;2-6 10.1002/1521-3994(200008)321:3<181::AID-ASNA181>3.0.CO;2-6zbMath0965.76028OpenAlexW2016012308MaRDI QIDQ4504341

Günther Rüdiger, L. L. Kitchatinov

Publication date: 21 November 2000

Full work available at URL: https://doi.org/10.1002/1521-3994(200008)321:3<181::aid-asna181>3.0.co;2-6

zbMATH Keywords

critical temperatureringsmarginal stabilityplanetary systemsgravitational instabilityaccretion disksprotoplanetary disksforming planetsglobal linear analysisglobal nonaxisymmetric vorticesone-armed trailing spiralsself-gravitating infinitesimally thin gaseous disk

Mathematics Subject Classification ID

Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Stability and instability of geophysical and astrophysical flows (76E20) Astrophysical cosmology (85A40)

Cites Work

• Unnamed Item
• On the Stability of Differentially Rotating Bodies

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