Differential rotation and hydrodynamic stability of hot neutron stars

Astronomy and Astrophysics

Volumn 408, Issue 1, 2003, Pages 331-335

  Urpin, V ^a,b  

^a IOFFE INSTITUTE   (Russian Federation)

^b Isaak Newton Institute of Chili   (Russian Federation)

Author keywords

MHD; Stars: Neutron; Stars: Pulsars: General; Stars: Rotation

Indexed keywords

APPROXIMATION THEORY; GALAXIES; MAGNETOHYDRODYNAMICS; ORBITS; PERTURBATION TECHNIQUES; STABILITY; THERMAL DIFFUSION IN GASES; VISCOSITY OF GASES;

BINARY NEUTRON STAR; BOUSSINESQ APPROXIMATION; DIFFERENTIAL ROTATION; HYDRODYNAMIC INSTABILITY; THERMAL DIFFUSIVITY; YOUNG NEUTRON STAR;

ASTRONOMY;

EID: 0041693912     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20030917     Document Type: Article

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