Stellar Evolution Tracks
   
  
  
   
      J.Köppen Strasbourg/Illkirch/Kiel May 2001
   
  
  
 
 
  The StellarEvolution Applet displays
  the properties of stars of different masses and for different ages.
  The screen is organized in a plotting area and some control butttons: 
  
      
  
  The controls on the top are:
  
    -  Clear wipes the plot
    
 -  X= and Y= allow to select which parameter is 
         to be plotted as abscissa and ordinate. The parameters are:
         effective temperature, luminosity, radius, mass, surface
         gravity, age (either linear or logarithmic), phoptometric
         colours U, B, V, and colour indices U-B and B-V.
    
 -  drag & zoom after clicking the button, drag the mouse
         over a rectangle in the plot area. After releasing the mouse
         the plot will be zommed into this rectangle
    
 -  unZoom restores the full view
  
 
  The controls on the side are:
  
    -  Z=0.02 allows to select the metallicity of the stars
        between 0.001, 0.004, 0.008, 0.02 (solar), and 0.04       
    
 -  Mass enter the stellar mass in the text field (in solar units)
    
 -  Evolutionary Track will draw the track of a star of this
        mass as a black curve, from zero age to the specified maximum age 
    
 -  Age enter the age in the text field (in Gyr)
    
 -  Isochrone draws the positions of stars of any mass but
        of the specified age as a red curve
    
 -  Star draws the position of the star of given mass and
        age as a small black dot, and its effective temperature and luminosity
        are displayed in the field below. Note: if no dot appears, the star has
        already finished its life.
  
 
  Clicking on the plotting area will cause the x and y coordinates being
  displayed above the plot.
  
  
   These evolutionary tracks are results of computations for spherically
   symmetric, non-rotating stars by the Geneva group. 
   Note that they do not include the evolution beyond the
   red giant branch: the ascent up the asymptotic giant branch
   (AGB), evolution from AGB to white dwarfs, cooling sequence of white
   dwarfs, and the horizontal branch are not shown here.
   
  
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