Lagrangian perturbation theory of non-relativistic rotating superfluid stars

Monthly Notices of the Royal Astronomical Society

Volumn 355, Issue 3, 2004, Pages 918-928

  Andersson, N ^a   Comer, G L ^b   Grosart, K ^a  

^a UNIVERSITY OF SOUTHAMPTON   (United Kingdom)

^b Saint Louis University   (United States)

Author keywords

Gravitational waves; Hydrodynamics; Instabilities; Stars: neutron

Indexed keywords

HYDRODYNAMICS; LAGRANGE MULTIPLIERS; NEUTRONS; PERTURBATION TECHNIQUES; STARS; TWO PHASE FLOW;

GENERALISATION; LAGRANGIAN; NEUTRON STARS; PERTURBATION THEORY; RELATIVISTICS; ROTATING STARS; STABILITY PROPERTIES; STARS: NEUTRONS; SUPERFLUID COMPONENT; TWO-FLUID MODELING;

STABILITY;

EID: 10844244057     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2004.08370.x     Document Type: Article

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