Stefan Keller
Research Fellow, Research School of Astronomy and Astrophysics, Australian National University
Stellar Evolution Research
 
3d Radiative Hydrodynamical Model
 
Djehuty - the first 3d radiative hydro code of a stellar interior.
Thesis Studies of Young Populous Clusters Within the Magellanic Clouds
 
I finished my thesis at Mt. Stromlo Observatory, ANU, Australia in Sept. 2000. I analysed data obtained with the WFPC2 camera on board the HST. We have observed the clusters NGC 330, 1818, 2004, 2100. Results are presented in our AJ paper. From a comparison of the observed data set and that simulated from the stellar evolutionary models we conclude that the case of no convective core overshoot is excluded at a 2 sigma level.
 
Stefan Keller Contact Details ANU RSAA (Mt. Stromlo) SkyMapper Research Hyper - The First Stars Galactic Structure Stellar Pulsation Stellar Evolution 3D Stellar Modelling Institute of Geophysics and Planetary Physics The MACHO Project The SuperMACHO Project MCOrigins - Magellanic Clouds Program Teaching Stefan%20Keller.htmlContact.htmlhttp://www.anu.edu.au/http://www.mso.anu.edu.au/http://www.mso.anu.edu.au/~stefan/skymapperHyper.htmlHalo%20Structure.htmlStellar%20Pulsation.htmlhttp://www.llnl.gov/str/May02/Dearborn.htmlhttp://www.llnl.gov/urp/IGPP/http://wwwmacho.mcmaster.ca/http://www.phys.washington.edu/~stubbs/MCOrigins.htmlTeaching.htmlhttp://msowww.anu.edu.au/~wood/Lectures.htmlshapeimage_2_link_0shapeimage_2_link_1shapeimage_2_link_2shapeimage_2_link_3shapeimage_2_link_4shapeimage_2_link_5shapeimage_2_link_6shapeimage_2_link_7shapeimage_2_link_8shapeimage_2_link_9shapeimage_2_link_10shapeimage_2_link_11shapeimage_2_link_12shapeimage_2_link_13shapeimage_2_link_14shapeimage_2_link_15