Strange stars as persistent sources of gravitational waves

Monthly Notices of the Royal Astronomical Society

Volumn 337, Issue 4, 2002, Pages 1224-1232

  Andersson, N ^a   Jones, D I ^a,b   Kokkotas, K D ^c  

^a UNIVERSITY OF SOUTHAMPTON   (United Kingdom)

^b PENNSYLVANIA STATE UNIVERSITY   (United States)

^c ARISTOTLE UNIVERSITY OF THESSALONIKI   (Greece)

Author keywords

Accretion, accretion discs; Radiation mechanisms: non thermal; Relativity; Stars: neutron; Stars: rotation

Indexed keywords

GRAVITATIONAL EFFECTS; GRAVITY WAVES; NEUTRONS; QUANTUM THEORY; RELATIVITY; SIGNAL DETECTION;

ACCRETION: ACCRETION DISKS; CLUSTERINGS; GRAVITATIONAL-WAVES; MODE INSTABILITIES; NEUTRON STARS; QUASI-EQUILIBRIUM STATE; RADIATION MECHANISMS: NONTHERMAL; STARS: NEUTRONS; STARS: ROTATION; TIME-SCALES;

STARS;

EID: 0043094320     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2002.05837.x     Document Type: Article

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