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Showing 1–2 of 2 results
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  • Type Ic supernovae (SNe) originate either from the core collapse of very massive stars or from less massive stars in binary systems. Here, the authors show that progenitors of Type II and Ic SNe have comparable lifetimes and initial masses, which supports binary interaction for most Type Ic SNe progenitors.

    • Martín Solar
    • Michał J. Michałowski
    • Radosław Wróblewski
    ResearchOpen Access
    Nature Communications
    Volume: 15, P: 1-9

  • A new class of ultra-long-duration γ-ray bursts (GRBs) has recently been suggested, with durations in excess of 10,000 seconds, and now a supernova (SN 2011kl) has been found to be associated with the ultra-long-duration GRB 111209A, allowing a physical understanding of the nature of ultra-long-duration GRBs.

    • Jochen Greiner
    • Paolo A. Mazzali
    • Karla Varela
    Research
    Nature
    Volume: 523, P: 189-192