Construction of highly accurate models of rotating neutron stars - Comparison of three different numerical schemes

Astronomy and Astrophysics Supplement Series

Volumn 132, Issue 3, 1998, Pages 431-454

  Nozawa, T ^a   Stergioulas, N ^b,d   Gourgoulhon, E ^c   Eriguchi, Y ^a  

^a UNIVERSITY OF TOKYO   (Japan)

^b UNIVERSITY OF WISCONSIN MILWAUKEE   (United States)

^c OBSERVATOIRE DE PARIS   (France)

^d ALBERT EINSTEIN INSTITUT   (Germany)

Author keywords

Methods: numerical; Pulsars: general; Relativity; Stars: neutron; Stars: rotation

Indexed keywords

EID: 33748549665     PISSN: 03650138     EISSN: None     Source Type: Journal    
DOI: 10.1051/aas:1998304     Document Type: Review

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