Asymmetry of Type IIP Supernovae

Details Asymmetry of Type IIP Supernovae Asymmetry of Type IIP Supernovae

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aipc..937..357c&link_type=abstract

SUPERNOVA 1987A: 20 YEARS AFTER: Supernovae and Gamma-Ray Bursters. AIP Conference Proceedings, Volume 937, pp. 357-364 (2007).

Computer Science

2

Supernovae, Supernova Remnants, Magnetic And Electric Fields, Polarization Of Starlight

Scientific paper

Data on SN 1987A asymmetry are reviewed and summarized in the statement that its asphericity is caused by bipolar 56Ni ejecta with asymmetric jets. I present convincing evidence that in normal type IIP supernovae we also see the asymmetry caused by asymmetric bipolar 56Ni jets. Yet a significant fraction of 56Ni resides in the central symmetric component. The major conclusion is that the violation of the point symmetry is a generic property of the SN IIP explosion mechanism.

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