The Home Page of Mike Montgomery

The Home Page of Mike Montgomery

Job Related Links

Curriculum Vitae (pdf, ps)
Publication List (html, pdf, ps)
Description of Research (pdf, ps)

Research

Stellar Structure and Evolution Stellar Pulsation Arxived Preprints
Dissertation (pdf, ps)
Master's thesis (pdf, ps)

Lecture Notes

Scientific Talks

Public Lectures

Music

Pictures

Address

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)

This middle panel of this plot shows the fit (red curve) to the observed pulseshape (black curve) for the star G29-38; this fit is achieved by varying the convective parameters, the amplitude and phase of the mode, and the inclination angle. In the upper panel, we see that the derived thermal response timescale of the convection zone (red curve) is very similar to that which one calculates from standard mixing-length theory (black curve). For a movie of this solution, click here.




Michael H. Montgomery, mikemon@astro.as.utexas.edu (1 Oct 2004)