Possible direct method to determine the radius of a star from the spectrum of gravitational wave signals

Physical Review Letters

Volumn 85, Issue 13, 2000, Pages 2665-2668

  Saijo, Motoyuki ^a   Nakamura, Takashi ^b  

^a WASEDA UNIVERSITY   (Japan)

^b KYOTO UNIVERSITY   (Japan)

Author keywords

[No Author keywords available]

Indexed keywords

ASTRONOMY; SPECTRUM ANALYSIS;

KERR BLACK HOLE;

GRAVITY WAVES;

EID: 0034714660     PISSN: 00319007     EISSN: 10797114     Source Type: Journal    
DOI: 10.1103/PhysRevLett.85.2665     Document Type: Article

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