Impact of the nuclear equation of state on the last orbits of binary neutron stars

Astronomy and Astrophysics

Volumn 431, Issue 1, 2005, Pages 297-306

  Bejger, M ^a   Gondek Rosinska D ^a,b   Gourgoulhon, E ^b   Haensel, P ^a,b   Taniguchi, K ^c,d   Zdunik, J L ^a  

^a NICOLAUS COPERNICUS ASTRONOMICAL CENTER   (Poland)

^b UNIVERSITÉ PARIS DIDEROT   (France)

^c UNIVERSITY OF TOKYO   (Japan)

^d University of Illinois at Urbana Champaign   (United States)

Author keywords

Binaries: close; Dense matter; Equation of state; Gravitational waves; Stars: neutron

Indexed keywords

APPROXIMATION THEORY; CALCULATIONS; FREQUENCIES; GRAVITY WAVES; HYDRODYNAMICS; MATHEMATICAL MODELS; ORBITS; RELATIVITY; TENSORS;

BINARIES: CLOSE; DENSE MATTER; EQUATION OF STATE; STARS: NEUTRON;

ASTROPHYSICS;

EID: 13844254264     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20041441     Document Type: Article

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