Massive Stellar Mergers as Precursors of Hydrogen-rich Pulsational Pair Instability Supernovae

25 Apr 2019 Vigna-Gómez Alejandro Justham Stephen Mandel Ilya de Mink Selma E. Podsiadlowski Philipp

Interactions between massive stars in binaries are thought to be responsible for much of the observed diversity of supernovae. As surveys probe rarer populations of events, we should expect to see supernovae arising from increasingly uncommon progenitor channels... (read more)

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  • HIGH ENERGY ASTROPHYSICAL PHENOMENA
  • SOLAR AND STELLAR ASTROPHYSICS