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Volumn 56, Issue 6, 1997, Pages 3416-3438

Post-Newtonian models of binary neutron stars

Author keywords

[No Author keywords available]

Indexed keywords


EID: 0000758809     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.56.3416     Document Type: Article
Times cited : (47)

References (54)
  • 24
    • 85038303626 scopus 로고
    • 432, 242 (1994);
    • (1994) , vol.432 , pp. 242
  • 28
    • 0004251401 scopus 로고
    • Frontiers in Numerical Relativity, edited by C. R. Evans, L. S. Finn, and D. W. Hobill (Cambridge University Press, Cambridge, England, 1989)
    • For earlier work, see articles in Sources of Gravitational Radiation, edited by L. Smarr (Cambridge University Press, Cambridge, 1979);and in Frontiers in Numerical Relativity, edited by C. R. Evans, L. S. Finn, and D. W. Hobill (Cambridge University Press, Cambridge, England, 1989).
    • (1979) Sources of Gravitational Radiation
  • 29
    • 0001456981 scopus 로고
    • For more recent progress, see R. A. Matzner et al. Science 270, 941 (1995).
    • (1995) Science , vol.270 , pp. 941
    • Matzner, R.A.1
  • 42
    • 84914783674 scopus 로고    scopus 로고
    • edited by S. Hawking and W. Israel (Cambridge University Press, Cambridge, 1987), p. 128
    • T. Damour, in 300 Years of Gravitation, edited by S. Hawking and W. Israel (Cambridge University Press, Cambridge, 1987), p. 128.
    • 300 Years of Gravitation
    • Damour, T.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.