Magnetorotational Collapse of Very Massive Stars: Formation of Jets and Black Holes

Details Magnetorotational Collapse of Very Massive Stars: Formation of Jets and Black Holes Magnetorotational Collapse of Very Massive Stars: Formation of Jets and Black Holes

Jul 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aipc..847..476s&link_type=abstract

ORIGIN OF MATTER AND EVOLUTION OF GALAXIES: International Symposium on Origin of Matter and Evolution of Galaxies 2005: New Hori

Astronomy and Astrophysics

Astrophysics

1

Population Iii Stars, Stellar Rotation, Magnetohydrodynamics And Plasmas, Black Holes

Scientific paper

Population III stars are thought to be very massive stars. However, their properties are not clarified yet. In this research, we investigate the features of magnetorotational dynamics of such stars with computer simulations. We find jet-like explosion in a few models and reveal what type of initial model undergo explosion. In addition, we inquire features of newborn black holes as a remnant of core-collapse.

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