Red supergiants are massive stars at the end of their lives. Theoretical predictions about how they go supernova have not matched observed data. In this podcast, Dr. Emma Beasor, a Hubble Fellow at NSF’s OIR Lab, discusses recent research that attempts to explain the red supergiant problem.

https://nationalastro.org/

Rob Sparks is a science education specialist in the EPO group at NOAO and works on the Galileoscope project (www.galileoscope.org), providing design, dissemination and professional development. He also pens a great blog at halfastro.wordpress.com.

 

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