On the relation between peak luminosity and parent population of Type Ia supernovae: A new tool for probing the ages of distant galaxies

We study the properties of Type Ia supernovae (SNe Ia) as functions of the radial distance from their host galaxy centers. Using a sample of 62 SNe Ia with reliable luminosity, reddening, and decline rate determinations, we f ind no significant radial gradients of SNe Ia peak absolute magnitudes or d ecline rates in elliptical + S0 galaxies, suggesting that the diversity of SN properties is not related to the metallicity of their progenitors. We do find that the range in brightness and light curve width of supernovae in s piral galaxies extends to brighter, broader values. These results are inter preted as support for an age, but not metallicity, related origin of the di versity in SNe Ia. If confirmed with a larger and more accurate sample of d ata, the age-luminosity relation would offer a new and powerful tool to pro be the ages and age gradients of stellar populations in galaxies at redshif t as high as z similar to 1-2. The absence of significant radial gradients in the peak (B - V)(0) and (V - I)(0) colors of SNe Ia supports the reddeni ng correction method of Phillips et al. We find no radial gradient in resid uals from the SN Ia luminosity-width relation, suggesting that the relation is not affected by properties of the progenitor populations and supporting the reliability of cosmological results based upon the use of SNe fa as di stance indicators.