Stellar Structure & Evolution, fall 2003
Written report and oral presentation

Steps

  1. Decide on a topic with Bengt.
  2. Search the library and the Web for suitable books and articles.
  3. Write and submit a report, with at least two A4 pages of text, on the chosen topic.
  4. Give the presentation to the entire class on October 28 or 30.
    Be sure to provide copies of your report for the other students.


Topics

Below is a list containing some possibilities to help you choose a topic for a presentation.
Feel free to discuss your own suggestions with Bengt!

Topic Taken by
The initial mass function (IMF)  
Star formation efficiencies in different environments  
Nuclear processes occurring on the main sequence  
Sunspots or magnetic fields in stars AP
Stellar rotation ML
Evolutionary effects on stars in binaries SN
Theoretical vs. observed H-R diagrams AB
Stellar evolution on the asymptotic giant branch (AGB)  
Novae KH
Processes in the core-collapse of massive stars EH
Processes in thermonuclear supernovae MS
Neutrinos from stars PT
Stellar winds  
...any other topic that has been checked with Bengt...  


Literature search

Speaking hints



Uppsala Astronomical Observatory
Department of Astronomy and Space Physics
Uppsala University
Box 515
SE-751 20 Uppsala
SWEDEN

Last modified: Tue Oct 7 14:40 MEST 2003
Corrections to: Michelle.Mizuno-Wiedner@astro.uu.se