Physics
Scientific paper
Aug 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006iaujd...9e..13g&link_type=abstract
Supernovae: One Millennium After SN1006, 26th meeting of the IAU, Joint Discussion 9, 17-18 August 2006, Prague, Czech Republic,
Physics
Scientific paper
Type Ia supernovae are believed to be thermonuclear explosions of carbon-oxygen white dwarf stars. Observationally they show a wide range of light curve shapes and peak luminosities at optical wavelengths. I discuss how type Ia supernova characteristics correlate with galaxy properties such as morphology, metallicity and star-formation rate. Also, I explore host properties at high and low redshift.
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