22 September 2005
22 September 2005
Speaker: Steven Stahler (UC Berkeley)
Title:Unsolved Problems in Star Formation
Abstract:
There are still major unsolved questions in the theory of star formation. How
do clusters form out of large molecular clouds? How do the disks around
individual stars accrete onto those objects?
In addressing such issues, theorists generally assume that processes occur on a
rapid (dynamical) time scale. Yet observations clearly demonstrate otherwise.
Dynamical proceses are easier to model numerically, but a quasi-static picture
is often more appropriate.
I discuss how this realization can help address the two specific problems of
cluster formation and disk accretion. In the latter area, fresh theoretical
ideas and the powerful capabilities of the SMA should lead to significant
progress in the near future.
Video of the Presentation
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