Magnetorotational collapse of population III stars

Publications of the Astronomical Society of Japan

Volumn 59, Issue 4, 2007, Pages 771-785

  Suwa, Yudai ^a   Takiwaki, Tomoya ^a   Kotake, Kei ^b   Sato, Katsuhiko ^a,c  

^a UNIVERSITY OF TOKYO   (Japan)

^b NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^c UNIVERSITY OF TOKYO   (Japan)

Author keywords

Black hole physics; Methods: numerical magnetohydrodynamics: MHD; Neutrinos; Stars: supernovae: general

Indexed keywords

BINDING ENERGY; BLACK HOLES; COSMOLOGY; EQUATIONS OF STATE; FIGHTER AIRCRAFT; GRAVITATION; LUMINANCE; NEUTRONS; NUMERICAL METHODS; ROTATION; SHOCK WAVES; SUPERNOVAE;

BLACK HOLE FORMATION; BLACK HOLE PHYSICS; COLLAPSE SIMULATION; CORE COLLAPSE; MAGNETIC-FIELD; METHOD: NUMERICAL; METHOD: NUMERICAL MAGNETOHYDRODYNAMIC: MHD; PROPERTY; STARS: SUPERNOVAE: GENERAL; TWO-DIMENSIONAL;

MAGNETOHYDRODYNAMICS;

EID: 34748907993     PISSN: 00046264     EISSN: None     Source Type: Journal    
DOI: 10.1093/pasj/59.4.771     Document Type: Article

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