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Pre-SN Mass-loss
  • Matteo Cantiello,
  • Raffaella Margutti,
  • Jeremiah Murphy
Matteo Cantiello
Kavli Institute for Theoretical Physics
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Raffaella Margutti
New York University (NYU)
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Jeremiah Murphy
Florida State University
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Our goal is to reconstruct pre-SN mass-loss history using radio variability observations and constrain the dominant mass-loss mechanism during the last few hundred years of massive star evolution. We will draw from existing observations to re-design the strategy for future observing campaigns.