TL;DR
This paper explores the mass ranges of type IIP supernova progenitors, implications for stellar evolution, and examines specific supernovae to infer properties of Wolf-Rayet stars and gamma-ray bursts.
Contribution
It provides new insights into the mass limits of supernova progenitors and their relation to stellar evolution and explosive phenomena.
Findings
Constraints on stellar evolution from supernova progenitor mass ranges
Implications for Wolf-Rayet star mass-loss rates
Connections between supernovae and gamma-ray bursts
Abstract
We first discuss the mass range of type IIP SN progenitors and how the upper and lower limits impose interesting constraints on stellar evolution. Then we discuss the possible implications of two SNe, 2002ap and 2006jc, for Wolf-Rayet star mass-loss rates and long Gamma-ray bursts.
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