Bipolar explosion models for hypernovae

Details Bipolar explosion models for hypernovae Bipolar explosion models for hypernovae

May 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003nupha.718..167m&link_type=abstract

Nuclear Physics A, Volume 718, p. 167-170.

Physics

Nuclear Physics

4

Scientific paper

Bipolar explosion models for hypernovae (very energetic supernovae) are presented. These models provide a favorable situation to explain some unexpected features in observations of hypernovae, e.g., high velocity matter dominated by Fe and low velocity matter dominated by O. The overall abundance of these models gives a good fit, at least qualitatively, to abundances in extremely metal-poor stars. We suggest hypernovae be driven by bipolar jets and contribute significantly to the early Galactic chemical evolution.

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