Lagrangian perturbation theory for rotating magnetic stars

Monthly Notices of the Royal Astronomical Society

Volumn 377, Issue 2, 2007, Pages 630-644

  Glampedakis, Kostas ^a   Andersson, Nils ^a  

^a UNIVERSITY OF SOUTHAMPTON   (United Kingdom)

Author keywords

Hydrodynamics; Instabilities; MHD; Stars: magnetic fields; Stars: neutron

Indexed keywords

LAGRANGE MULTIPLIERS; PERTURBATION TECHNIQUES; STABILITY CRITERIA; STARS;

ENERGY; FLUID DISPLACEMENT; LAGRANGIAN; LINEAR PERTURBATIONS; MAGNETIC-FIELD; PERTURBATION THEORY; STABILITY CRITERIONS; STABILITY PROPERTIES; STARS: MAGNETIC FIELD; STARS: NEUTRONS;

MAGNETOHYDRODYNAMICS;

EID: 34247627886     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2007.11625.x     Document Type: Article

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