A quasi-radial stability criterion for rotating relativistic stars

Monthly Notices of the Royal Astronomical Society: Letters

Volumn 416, Issue 1, 2011, Pages

  Takami, Kentaro ^a   Rezzolla, Luciano ^a,b   Yoshida, Shin'ichirou ^c  

^a ALBERT EINSTEIN INSTITUT   (Germany)

^b LOUISIANA STATE UNIVERSITY   (United States)

^c UNIVERSITY OF TOKYO   (Japan)

Author keywords

Black hole physics; Methods: numerical; Relativistic processes; Stars: neutron; Stars: oscillations; Stars: rotation

Indexed keywords

EID: 84055198558     PISSN: 17453933     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1745-3933.2011.01085.x     Document Type: Article

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