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Browsing by Subject "Stellar oscillations -- Mathematical models"
Now showing items 1-4 of 4
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(Halifax, N.S. : Saint Mary's University, 2003)Stellar non-radial oscillations (p-modes) are ideal tools to test theories of stellar evolution and to provide information about stellar properties. This thesis develops and tests a technique to determine the stellar model ...
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(Halifax, N.S. : Saint Mary's University, 2013)We have developed a three-dimensional radiation hydrodynamics code to simulate the interaction of convection and pulsation in classical variable stars. One key goal is the ability to carry these simulations to full amplitude ...
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(Halifax, N.S. : Saint Mary's University, 2016)In this thesis I present a set of scaling relationships for ZAMS rotating models. These relationships are applicable to models whose rotation rate produces a given surface distortion and are shown to be valid for stellar ...
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(Halifax, N.S. : Saint Mary's University, 1996)The mixing length parameter is a free parameter governing convective energy transport in current stellar models, and is poorly constrained by current photometric observations. Theoretical nonradial pulsation spectra have ...
Now showing items 1-4 of 4