Numerical study on the hydrodynamic instability of binary stars in the first post Newtonian approximation of general relativity

Progress of Theoretical Physics

Volumn 98, Issue 5, 1997, Pages 1081-1098

  Shibata, Masaru ^a   Oohara, Ken Ichi ^b   Nakamura, Takashi ^c  

^a OSAKA UNIVERSITY   (Japan)

^b NIIGATA UNIVERSITY   (Japan)

^c KYOTO UNIVERSITY   (Japan)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0031322483     PISSN: 0033068X     EISSN: None     Source Type: Journal    
DOI: 10.1143/PTP.98.1081     Document Type: Article

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