Type II Supernovae: from Under-luminous to Hyper-luminous

Details Type II Supernovae: from Under-luminous to Hyper-luminous Type II Supernovae: from Under-luminous to Hyper-luminous

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1111..249z&link_type=abstract

PROBING STELLAR POPULATIONS OUT TO THE DISTANT UNIVERSE: CEFALU 2008, Proceedings of the International Conference. AIP Conferen

Physics

1

Supernova Remnants, Distances, Redshifts, Radial Velocities, Spatial Distribution Of Galaxies, Star Formation

Scientific paper

We present recent results on two Type II supernovae (SNe) with rather extreme properties, the low luminosity SN 2005 ay and the very bright Type IIn SN 2006 gy. They lie at the opposite tails of the luminosity distribution of Type II SNe and provide us with invaluable information on the physical properties of these events and their connection with their progenitor systems.

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