The Home Page of Mike Montgomery

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

Teaching

Research

Stellar Structure and Evolution Stellar Pulsation Long Wavelength Array (LWA)

Arxived Preprints
Dissertation (pdf, ps)
Master's thesis (pdf, ps)

Lecture Notes

Scientific Talks

Public Lectures

Posters

Music

  • Hot Jazz Caravan
  • Hard To Make a Living
  • The Hemingford String Band
  • The Radio Cowboys
  • George Breakfast
  • Oliver Gruen
  • Nugget
  • Miscellaneous Pictures




  • Mike Montgomery
    Department of Astronomy
    University of Texas
    Austin, TX 78712
    USA

    mikemonastro.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.




    Last modified: Wed Nov 4 20:15:53 CST 2009