Friday, April 8, at 3:20 PM in NSC 224. Join us for refreshments in NSC 231 at 3:05 PM.
"How (and when) do stars lose mass?"
Dr. Lee Anne Willson, Iowa State University, Dept. of Physics and Astronomy
Our understanding of how stars and populations of stars evolve are mostly based
on models that assume constant mass. However, we also know that most stars lose
a considerable portion of their masses; for example, our Sun will end up as at
0.5 to 0.6 solar mass white dwarf. When and how do stars lose this mass, and
how do we know? Are widely used "empirical" mass loss formulae reliable - and
if so, why are they so varied in their prescriptions? I will review what we
know from observations about mass loss from stars, and describe what we have
learned recently about the mechanism(s) of mass loss for stars like the Sun when
they grow old.