Incompressible fluid binary systems with internal flows - Models of close binary neutron star systems with spin

Monthly Notices of the Royal Astronomical Society

Volumn 299, Issue 2, 1998, Pages 575-587

  Uryu, K ^a,b,c   Eriguchi, Y ^c  

^a ABDUS SALAM INTERNATIONAL CENTRE FOR THEORETICAL PHYSICS   (Italy)

^b SISSA   (Italy)

^c UNIVERSITY OF TOKYO   (Japan)

Author keywords

Binaries: close; Hydrodynamics; Instabilities; Stars: neutron; Stars: rotation

Indexed keywords

CRITICAL CURRENT DENSITY (SUPERCONDUCTIVITY); GRAVITY WAVES; NEUTRONS; STARS; SYSTEMS (METALLURGICAL);

BINARIES: CLOSE; BINARY NEUTRON STARS; BINARY SYSTEMS; INCOMPRESSIBLE FLUID; INTERNAL FLOWS; NEUTRON STARS; STAR SYSTEMS; STARS: BINARIES; STARS: NEUTRONS; STARS: ROTATION;

STABILITY;

EID: 0000181165     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.1998.01795.x     Document Type: Article

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