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A shallow-water theory for annular sections of Keplerian disks

Author
UMURHAN, O. M1 2 3
[1] Astronomy Unit, School of Mathematical Sciences, Queen Mary University of London, London El 4NS, United Kingdom
[2] Department of Geophysics and Space Sciences, Tel-Aviv University, Tel-Aviv, Israel
[3] Astronomy Department, City College of San Francisco, San Francisco, CA 94112, United States
Source

Astronomy and astrophysics (Berlin. Print). 2008, Vol 489, Num 3, pp 953-962, 10 p ; ref : 1/2 p

CODEN
AAEJAF
ISSN
0004-6361
Scientific domain
Astronomy earth cosmic environment
Publisher
EDP Sciences, Les Ulis
Publication country
France
Document type
Article
Language
English
Author keyword
circumstellar matter hydrodynamics instabilities waves
Keyword (fr)
Dynamique Ecoulement bidimensionnel Equation état Instabilité Lagrangien Matière circumstellaire Perturbation Polytrope Théorie asymptotique Tourbillon potentiel
Keyword (en)
Dynamics Two dimensional flow Equations of state Instability Lagrangian Circumstellar matter Disturbances Polytropes Asymptotic theory Potential vorticity
Keyword (es)
Flujo bidimensional Lagrangiano Vorticidad potencial
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
20714338

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS

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