The Home Page of Mike Montgomery
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Curriculum Vitae (pdf, ps)Publication List (html, pdf, ps)
Description of Research (pdf, ps)
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Stellar Structure and Evolution Stellar Pulsation Long Wavelength Array (LWA)Arxived Preprints
Dissertation (pdf, ps)
Master's thesis (pdf, ps)
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- Cambridge Astronomical Society
- Alston Hall Retreat
(talk1, talk2)
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Mike Montgomery
Department of Astronomy
University of Texas
Austin, TX 78712
USA
mikemon at astro.as.utexas.edu
+1 512 471 3451 (office)
+1 512 471 6417 (lab)
+1 512 471 6016 (fax)
+1 512 835 3425 (ARL)
+1 512 517 6753 (cell)
The black curve in the above plot shows data taken on the star GD 358 with the Nordic Telescope (NOT) in May/June 2006 in the recent WET/DARC run. The red curve is a 13-frequency fit to this data in which a time-dependent response of the convection zone has been included. The values of the convective parameters which were derived are tau = 447 sec, N = 25.3, and theta = 62 degrees. For a movie of this solution, click here.