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Physical Review Letters

Volumn 96, Issue 16, 2006, Pages

Formation of supermassive black holes through fragmentation of torodial supermassive stars

(6) Zink, Burkhard a Stergioulas, Nikolaos b Hawke, Ian c,d Ott, Christian D d Schnetter, Erik d,e Müller, Ewald a

a MAX PLANCK INSTITUT FÜR ASTROPHYSIK (Germany)

b ARISTOTLE UNIVERSITY OF THESSALONIKI (Greece)

c UNIVERSITY OF SOUTHAMPTON (United Kingdom)

d ALBERT EINSTEIN INSTITUT (Germany)

e LOUISIANA STATE UNIVERSITY (United States)

Author keywords

[No Author keywords available]

Indexed keywords

ADAPTIVE SYSTEMS; GRAVITATIONAL EFFECTS; ROTATION;

ADAPTIVE MESH REFINEMENT; NONAXISYMMETRIC MODES; ROTATING POLYTROPE; TORODIAL SUPERMASSIVE STARS;

ASTROPHYSICS;

EID: 33646369176 PISSN: 00319007 EISSN: 10797114 Source Type: Journal
DOI: 10.1103/PhysRevLett.96.161101 Document Type: Article

Times cited : (30)

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