Axisymmetric modes of rotating relativistic stars in the Cowling approximation

Monthly Notices of the Royal Astronomical Society

Volumn 325, Issue 4, 2001, Pages 1463-1470

  Font, José A ^a   Dimmelmeier, Harald ^a   Gupta, Anshu ^b   Stergioulas, Nikolaos ^c  

^a MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^b RAMAN RESEARCH INSTITUTE   (India)

^c ARISTOTLE UNIVERSITY OF THESSALONIKI   (Greece)

Author keywords

Hydrodynamics; Methods: numerical; Relativity; Stars: neutron; Stars: oscillations; Stars: rotation

Indexed keywords

FINITE DIFFERENCE METHOD; FOURIER SERIES; GRAVITATIONAL EFFECTS; GRAVITY WAVES; NUMERICAL METHODS; RELATIVITY; ROTATION RATE; STARS;

AXISYMMETRIC; AXISYMMETRIC MODES; COWLING APPROXIMATION; METHOD: NUMERICAL; NEUTRON STARS; RELATIVISTIC STARS; ROTATION RATE; STAR OSCILLATIONS; STARS: NEUTRONS; STARS: ROTATION;

HYDRODYNAMICS;

EID: 0001592124     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2001.04555.x     Document Type: Article

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