The Progenitor Masses Of Type IIP Supernovae From Late-time Spectral Modeling

Details The Progenitor Masses Of Type IIP Supernovae From Late-time Spectral Modeling The Progenitor Masses Of Type IIP Supernovae From Late-time Spectral Modeling

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012aas...21943602j&link_type=abstract

American Astronomical Society, AAS Meeting #219, #436.02

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Scientific paper

Type IIP supernovae (SNe) arise in the core-collapse of massive stars that have retained most of their hydrogen envelopes throughout their evolution. Progenitor analysis and hydrodynamical modeling have given strongly conflicting results for which type of stars are responsible for these explosions. We apply nebular-phase spectral modeling to diagnose the nucleosynthesis in these SNe, which is related to their progenitor ZAMS masses. I discuss results for the nearby SN 2004et as well as other Type IIP SNe.

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