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Stellar Structure and Evolution Stellar Pulsation Long Wavelength Array (LWA)ADS Abstracts
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- Cambridge Astronomical Society
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(talk1, talk2)
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Mike Montgomery
Department of Astronomy
University of Texas
Austin, TX 78712
USA
mikemon
astro.as.utexas.edu +1 512 471 3451 (office)
+1 512 471 6417 (lab)
+1 512 471 6016 (fax)
+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 12-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 = 611 sec, N = 23.8, and theta = 50.5 degrees. For a movie of this solution, click here.