Stellar Evolution with Pulsation-Driven Mass Loss: The Case of LMC   Cepheids
  The Cepheid mass discrepancy, the difference between mass estimates from stellar pulsation and stellar evolution models, is a long standing challenge for the understanding of stellar astrophysics. We discuss the current state of the mass discrepancy and test the role of pulsation-driven mass loss in state-of-the-art stellar evolution calculations of Large Magellanic Cepheids in resolving it. We find that Cepheid mass loss is a significant contributor to the mass discrepancy, but it is not clear if the metallicity dependence of Cepheid mass loss is consistent with the measured metallicity dependence of the mass discrepancy. 
Hilding Neilson (AIfA), Norbert Langer (AIfA), Matteo Cantiello (KITP,   AIfA)
astro-ph.SR