Measurement of the core-collapse progenitor mass distribution of the Small Magellanic Cloud

26 Nov 2018 Auchettl Katie Lopez Laura A. Badenes Carles Ramirez-Ruiz Enrico Beacom John F. Holland-Ashford Tyler

The physics of core-collapse (CC) supernovae (SNe) and how the explosions depend on progenitor properties are central questions in astronomy. For only a handful of SNe, the progenitor star has been identified in pre-explosion images... (read more)

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  • SOLAR AND STELLAR ASTROPHYSICS
  • ASTROPHYSICS OF GALAXIES
  • HIGH ENERGY ASTROPHYSICAL PHENOMENA