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University of Birmingham > Talks@bham > Physics and Astronomy Colloquia > Internal Gravity Waves in Massive Stars
Internal Gravity Waves in Massive StarsAdd to your list(s) Download to your calendar using vCal
If you have a question about this talk, please contact Yeshpal Singh. Internal Gravity Waves (IGW) propagate in the radiative regions of all stars. Within stars with convective cores and radiative envelopes these waves can play an important role in the rotational and chemical evolution of these stars. In this talk I will discuss work my group has done to understand these waves, the role they play in stars and how we might model them better in stellar evolution models so that we can better contextualise observations This talk is part of the Physics and Astronomy Colloquia series. This talk is included in these lists:Note that ex-directory lists are not shown. |
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