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Volumn 296, Issue 1, 1998, Pages
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Stationary states of irrotational binary neutron star systems and their evolution as a result of gravitational wave emission
a,b,c c |
Author keywords
Binaries: close; Hydrodynamics; Instabilities; Stars: neutron; Stars: rotation
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Indexed keywords
ANGULAR VELOCITY;
EQUATIONS OF STATE;
GRAVITATIONAL EFFECTS;
GRAVITY WAVES;
NEUTRONS;
STARS;
BINARIES: CLOSE;
BINARY NEUTRON STARS;
BINARY SYSTEMS;
CONTACT PHASE;
GRAVITATIONAL-WAVE EMISSION;
IRROTATIONAL;
NEUTRON STARS;
STARS: NEUTRONS;
STARS: ROTATION;
STATIONARY STATE;
SYSTEMS (METALLURGICAL);
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EID: 0002591772
PISSN: 00358711
EISSN: None
Source Type: Journal
DOI: 10.1046/j.1365-8711.1998.01385.x Document Type: Article |
Times cited : (20)
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References (24)
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